The complex circumstellar environment of supernova 2023ixf.

The early evolution of a supernova (SN) can reveal information about the environment and the progenitor star. When a star explodes in vacuum, the first photons to escape from its surface appear as a brief, hours-long shock-breakout flare1,2, followed by a cooling phase of emission. However, for stars exploding within a distribution of dense, optically thick circumstellar material (CSM), the first photons escape from the material beyond the stellar edge and the duration of the initial flare can extend to several days, during which the escaping emission indicates photospheric heating3. Early serendipitous observations2,4 that lacked ultraviolet (UV) data were unable to determine whether the early emission is heating or cooling and hence the nature of the early explosion event. Here we report UV spectra of the nearby SN 2023ixf in the galaxy Messier 101 (M101). Using the UV data as well as a comprehensive set of further multiwavelength observations, we temporally resolve the emergence of the explosion shock from a thick medium heated by the SN emission. We derive a reliable bolometric light curve that indicates that the shock breaks out from a dense layer with a radius substantially larger than typical supergiants.

An outburst from a massive star 40 days before a supernova explosion.

Some observations suggest that very massive stars experience extreme mass-loss episodes shortly before they explode as supernovae, as do several models. Establishing a causal connection between these mass-loss episodes and the final explosion would provide a novel way to study pre-supernova massive-star evolution. Here we report observations of a mass-loss event detected 40 days before the explosion of the type IIn supernova SN 2010mc (also known as PTF 10tel). Our photometric and spectroscopic data suggest that this event is a result of an energetic outburst, radiating at least 6 × 10(47) erg of energy and releasing about 10(-2) solar masses of material at typical velocities of 2,000 km s(-1). The temporal proximity of the mass-loss outburst and the supernova explosion implies a causal connection between them. Moreover, we find that the outburst luminosity and velocity are consistent with the predictions of the wave-driven pulsation model, and disfavour alternative suggestions.

Characterization of Influenza B Virus Variants with Reduced Neuraminidase Inhibitor Susceptibility.

Treatment options for influenza B virus infections are limited to neuraminidase inhibitors (NAIs), which block the neuraminidase (NA) glycoprotein on the virion surface. The development of NAI resistance would therefore result in a loss of antiviral treatment options for influenza B virus infections. This study characterized two contemporary influenza B viruses with known resistance-conferring NA amino acid substitutions, D197N and H273Y, detected during routine surveillance. The D197N and H273Y variants were characterized in vitro by assessing NA enzyme activity and affinity, as well as replication in cell culture compared to those of NAI-sensitive wild-type viruses. In vivo studies were also performed in ferrets to assess the replication and transmissibility of each variant. Mathematical models were used to analyze within-host and between-host fitness of variants relative to wild-type viruses. The data revealed that the H273Y variant had NA enzyme function similar to that of its wild type but had slightly reduced replication and transmission efficiency in vivo The D197N variant had impaired NA enzyme function, but there was no evidence of reduction in replication or transmission efficiency in ferrets. Our data suggest that the influenza B virus variant with the H273Y NA substitution had a more notable reduction in fitness compared to wild-type viruses than the influenza B variant with the D197N NA substitution. Although a D197N variant is yet to become widespread, it is the most commonly detected NAI-resistant influenza B virus in surveillance studies. Our results highlight the need to carefully monitor circulating viruses for the spread of influenza B viruses with the D197N NA substitution.

Genetic screening reveals a link between Wnt signaling and antitubulin drugs.

The antitubulin drugs, paclitaxel (PX) and colchicine (COL), inhibit cell growth and are therapeutically valuable. PX stabilizes microtubules, while COL promotes their depolymerization. But, the drug concentrations that alter tubulin polymerization are hundreds of times higher than their clinically useful levels. To map genetic targets for drug action at single-gene resolution, we used a human radiation hybrid panel. We identified loci that affected cell survival in the presence of five compounds of medical relevance. For PX and COL, the zinc and ring finger 3 (ZNRF3) gene dominated the genetic landscape at therapeutic concentrations. ZNRF3 encodes an R-spondin regulated receptor that inhibits Wingless/Int (Wnt) signaling. Overexpression of the ZNRF3 gene shielded cells from antitubulin drug action, while small interfering RNA knockdowns resulted in sensitization. Further a potent pharmacological inhibitor of Wnt signaling, Wnt-C59, protected cells from PX and COL. Our results suggest that the antitubulin drugs perturb microtubule dynamics, thereby influencing Wnt signaling.

Methamphetamine-associated cardiomyopathy: patterns and predictors of recovery.

BACKGROUND: Methamphetamine abuse is a growing public health problem, and increasing numbers of patients are admitted with methamphetamine-associated cardiomyopathy (MAC). AIM: We sought to characterise the patterns of this disease and identify predictors of recovery. METHODS: We retrospectively studied consecutive patients diagnosed with MAC between January 2006 and July 2015. RESULTS: We identified 20 patients (14 males, 6 females) with mean age 35 ± 9 years. Most had very severe systolic dysfunction (mean left ventricular ejection fraction (LVEF) 19.7 ± 11.4%) at presentation with 14 requiring inotropes and 5 requiring mechanical support. The pattern of systolic dysfunction was global in 14 patients, while 6 patients had a 'reverse Takotsubo' (RT) pattern with severely hypokinetic basal-mid segments and apical preservation. RT patients were predominantly female, had a short history of methamphetamine abuse and had higher cardiac enzyme levels. Patients with global dysfunction tended to have mid-wall fibrosis on cardiac magnetic resonance imaging. On follow-up transthoracic echocardiography, 6 out of 19 (32%) had normalisation of LVEF (LVEF ≥ 50%) within 6 weeks. Smaller left ventricular and left atrial size, shorter duration of methamphetamine use and RT pattern appeared to predict early recovery. CONCLUSION: A subset of MAC patients, particularly those with a RT pattern and lesser ventricular dilatation have the potential for early recovery of ventricular function. By contrast, those with evidence of myocardial fibrosis and ventricular enlargement have limited scope for recovery.

Supernova 2007bi as a pair-instability explosion.

Stars with initial masses such that 10M[symbol: see text] or= 140M[symbol: see text] (if such exist) develop oxygen cores with masses, M(core), that exceed 50M[symbol: see text], where high temperatures are reached at relatively low densities. Conversion of energetic, pressure-supporting photons into electron-positron pairs occurs before oxygen ignition and leads to a violent contraction which triggers a nuclear explosion that unbinds the star in a pair-instability supernova. Transitional objects with 100M[symbol: see text] < M(initial) < 140M[symbol: see text] may end up as iron-core-collapse supernovae following violent mass ejections, perhaps as a result of brief episodes of pair instability, and may already have been identified. Here we report observations of supernova SN 2007bi, a luminous, slowly evolving object located within a dwarf galaxy. We estimate the exploding core mass to be M(core) approximately 100M[symbol: see text], in which case theory unambiguously predicts a pair-instability supernova. We show that >3M[symbol: see text] of radioactive (56)Ni was synthesized during the explosion and that our observations are well fitted by models of pair-instability supernovae. This indicates that nearby dwarf galaxies probably host extremely massive stars, above the apparent Galactic stellar mass limit, which perhaps result from processes similar to those that created the first stars in the Universe.

A gamma-ray burst at a redshift of z approximately 8.2.

Long-duration gamma-ray bursts (GRBs) are thought to result from the explosions of certain massive stars, and some are bright enough that they should be observable out to redshifts of z > 20 using current technology. Hitherto, the highest redshift measured for any object was z = 6.96, for a Lyman-alpha emitting galaxy. Here we report that GRB 090423 lies at a redshift of z approximately 8.2, implying that massive stars were being produced and dying as GRBs approximately 630 Myr after the Big Bang. The burst also pinpoints the location of its host galaxy.

An infrared flash contemporaneous with the gamma-rays of GRB 041219a.

The explosion that results in a cosmic gamma-ray burst (GRB) is thought to produce emission from two physical processes: the central engine gives rise to the high-energy emission of the burst through internal shocking, and the subsequent interaction of the flow with the external environment produces long-wavelength afterglows. Although observations of afterglows continue to refine our understanding of GRB progenitors and relativistic shocks, gamma-ray observations alone have not yielded a clear picture of the origin of the prompt emission nor details of the central engine. Only one concurrent visible-light transient has been found and it was associated with emission from an external shock. Here we report the discovery of infrared emission contemporaneous with a GRB, beginning 7.2 minutes after the onset of GRB 041219a (ref. 8). We acquired 21 images during the active phase of the burst, yielding early multi-colour observations. Our analysis of the initial infrared pulse suggests an origin consistent with internal shocks.

Inversion Recovery Ultrashort TE MR Imaging of Myelin is Significantly Correlated with Disability in Patients with Multiple Sclerosis.

BACKGROUND AND PURPOSE: MR imaging has been widely used for the noninvasive evaluation of MS. Although clinical MR imaging sequences are highly effective in showing focal macroscopic tissue abnormalities in the brains of patients with MS, they are not specific to myelin and correlate poorly with disability. We investigated direct imaging of myelin using a 2D adiabatic inversion recovery ultrashort TE sequence to determine its value in assessing disability in MS. MATERIALS AND METHODS: The 2D inversion recovery ultrashort TE sequence was evaluated in 14 healthy volunteers and 31 patients with MS. MPRAGE and T2-FLAIR images were acquired for comparison. Advanced Normalization Tools were used to correlate inversion recovery ultrashort TE, MPRAGE, and T2-FLAIR images with disability assessed by the Expanded Disability Status Scale. RESULTS: Weak correlations were observed between normal-appearing white matter volume (R = -0.03, P = .88), lesion load (R = 0.22, P = .24), and age (R = 0.14, P = .44), and disability. The MPRAGE signal in normal-appearing white matter showed a weak correlation with age (R = -0.10, P = .49) and disability (R = -0.19, P = .31). The T2-FLAIR signal in normal-appearing white matter showed a weak correlation with age (R = 0.01, P = .93) and disability (R = 0.13, P = .49). The inversion recovery ultrashort TE signal was significantly negatively correlated with age (R = -0.38, P = .009) and disability (R = -0.44; P = .01). CONCLUSIONS: Direct imaging of myelin correlates with disability in patients with MS better than indirect imaging of long-T2 water in WM using conventional clinical sequences.

Paediatric endophthalmitis: a UK retrospective study.

INTRODUCTION: Paediatric endophthalmitis is a severe but rare complication of intraocular surgery, penetrating trauma and far less commonly extra-ocular surgery or endogenous origin. We set out to establish the incidence and risk factors of exogenous endophthalmitis in children, and to develop an evidence-based protocol that can be used for treatment of suspected exogenous endophthalmitis in children. METHODS: Microbiology reports and operation numbers were obtained from two large tertiary referral hospitals sharing 24-h paediatric ophthalmology cover for the period January 2009-December 2016. All cases of aqueous and/or vitreous tap performed on children aged ≤18 years were identified and case notes reviewed for complete information on each case. RESULTS: Sixteen cases were eligible for inclusion as 'postoperative endophthalmitis': complete data was found on 13 cases. The incidence of postoperative endophthalmitis was 0.17% over 7 years. The mean age of presentation was 5.5 years (range from 7 months to 16 years and 9 months), from 3 days-78 months post operatively. In all, 11/13 had at least one glaucoma procedure. Microbiology results showed growth in 8/13. Most isolates were Gram-positive bacteria but Gram-negatives were also isolated and in one case Candida from a conjunctival swab. The antibiotic regime varied depending on age, organism identified and sensitivities. In all, 9/13 had hand movement or worse vision after treatment. CONCLUSION: Paediatric endophthalmitis may present to any paediatric/general ophthalmologist. It is a rare but devastating condition with poor visual prognosis, requiring prompt recognition and aggressive management. Previous glaucoma surgery is a long-term risk factor in our local paediatric population. Based on our study, an evidence-based protocol for management is proposed in order to improve outcomes.

Tsukuba science city: Japan tries planned innovation.

Tsukuba Science City is Japan's new municipal complex of research laboratories and educational facilities. About 30 percent of the nation's government research laboratories and more than 40 percent of its government research manpower are concentrated in the community. A brief history of the monumental project is presented and problems confronting the city are discussed.

Germline genome protection: implications for gamete quality and germ cell tumorigenesis.

BACKGROUND: Germ cells have a unique and critical role as the conduit for hereditary information and therefore employ multiple strategies to protect genomic integrity and avoid mutations. Unlike somatic cells, which often respond to DNA damage by arresting the cell cycle and conducting DNA repair, germ cells as well as long-lived pluripotent stem cells typically avoid the use of error-prone repair mechanisms and favor apoptosis, reducing the risk of genetic alterations. Testicular germ cell tumors, the most common cancers of young men, arise from pre-natal germ cells. OBJECTIVES: To summarize the current understanding of DNA damage response mechanisms in pre-meiotic germ cells and to discuss how they impact both the origins of testicular germ cell tumors and their remarkable responsiveness to genotoxic chemotherapy. MATERIALS AND METHODS: We conducted a review of literature gathered from PubMed regarding the DNA damage response properties of testicular germ cell tumors and the germ cells from which they arise, as well as the influence of these mechanisms on therapeutic responses by testicular germ cell tumors. RESULTS AND DISCUSSION: This review provides a comprehensive evaluation of how the developmental origins of male germ cells and their inherent germ cell-like DNA damage response directly impact the development and therapeutic sensitivity of testicular germ cell tumors. CONCLUSIONS: The DNA damage response of germ cells directly impacts the development and therapeutic sensitivity of testicular germ cell tumors. Recent advances in the study of primordial germ cells, post-natal mitotically dividing germ cells, and pluripotent stem cells will allow for new investigations into the initiation, progression, and treatment of testicular germ cell tumors.

Bidirectional amyloid fiber growth for a yeast prion determinant.

The polymerization of many amyloids is a two-stage process initiated by the formation of a seeding nucleus or protofibril. Soluble protein then assembles with these nuclei to form amyloid fibers. Whether fiber growth is bidirectional or unidirectional has been determined for two amyloids. In these cases, bidirectional growth was established by time lapse atomic-force microscopy. Here, we investigated the growth of amyloid fibers formed by NM, the prion-determining region of the yeast protein Sup35p. The conformational changes in NM that lead to amyloid formation in vitro serve as a model for the self-perpetuating conformational changes in Sup35p that allow this protein to serve as an epigenetic element of inheritance in vivo. To assess the directionality of fiber growth, we genetically engineered a mutant of NM so that it contained an accessible cysteine residue that was easily labeled after fiber formation. The mutant protein assembled in vitro with kinetics indistinguishable from those of the wild-type protein and propagated the heritable genetic trait [PSI(+)] with the same fidelity. In reactions nucleated with prelabeled fibers, unlabeled protein assembled at both ends. Thus, NM fiber growth is bidirectional.

Illuminating gravitational waves: A concordant picture of photons from a neutron star merger.

Merging neutron stars offer an excellent laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart (EM170817) with gravitational waves (GW170817) detected from merging neutron stars. By synthesizing a panchromatic data set, we demonstrate that merging neutron stars are a long-sought production site forging heavy elements by r-process nucleosynthesis. The weak gamma rays seen in EM170817 are dissimilar to classical short gamma-ray bursts with ultrarelativistic jets. Instead, we suggest that breakout of a wide-angle, mildly relativistic cocoon engulfing the jet explains the low-luminosity gamma rays, the high-luminosity ultraviolet-optical-infrared, and the delayed radio and x-ray emission. We posit that all neutron star mergers may lead to a wide-angle cocoon breakout, sometimes accompanied by a successful jet and sometimes by a choked jet.

Social support and cancer screening among older black Americans.

BACKGROUND: Age-adjusted cancer mortality is 27% higher for Black Americans than for the general U.S. population, which may result from inappropriate use of cancer detection tests. Social support has been shown to affect adjustment to breast cancer and survival, but it has not been studied as a predictor of use of preventive health care services in the older population. Our hypothesis is that larger social networks are associated with greater utilization of cancer-screening tests in the older population. PURPOSE: The objective of this study was to examine the relationship between social support and use of cancer-screening tests among older Black Americans. METHODS: Data for this study were obtained from a 1986 baseline survey evaluation of a community intervention program to increase cancer awareness and a 1991 end-point survey of use of cancer detection tests. Our study sample consisted of 617 Black Americans aged 55 years or older who lived in San Francisco (Calif.), the control community, and in Oakland (Calif.), the target community for intervention. The survey included measures of 1) social network characteristics, as determined by a modified version of Berkman and Syme's Social Network Index; 2) demographic characteristics; and 3) use of six cancer-screening tests--mammography, occult blood stool examination, cervical smear, clinical breast examination, digital rectal examination, and sigmoidoscopy. RESULTS: Multiple logistic regression analysis of the Social Network Index results indicated statistically significant positive associations of social support with the use of mammography and occult blood stool examination but not with the other cancer-screening tests. There were statistically significant associations between having HMO (Health Maintenance Organization) insurance and increased use of mammography and occult blood stool examination, compared with having Medi-Cal or other insurance. The interval between the surveys had a statistically significant positive association with use of mammography. These significant associations were not explained by differences in the other variables, which included health status, age, gender, education, type of health insurance, interval between the surveys, and a regular source of care. CONCLUSIONS: Social support seems to be associated with increased use of mammography and occult blood stool examinations among older Black Americans. IMPLICATIONS: Interventions designed to increase utilization of social networks may be an effective way to increase use of cancer screening, which may ultimately lead to reduced mortality from cancer.

Glucocorticoid receptors in peripheral blood lymphocytes from bovine leukemia virus-infected cows with persistent lymphocytosis.

Bovine leukemia virus-infected cows with persistent lymphocytosis have an expanded population of B-lymphocytes in the peripheral blood that is sensitive to glucocorticoids in vitro and in vivo. We examined peripheral blood lymphocytes from cows with persistent lymphocytosis for the presence of specific glucocorticoid receptors. Steroid binding in intact cells was determined by a whole cell competitive binding assay using [3H]dexamethasone. The binding of the glucocorticoid to receptor was characterized in terms of affinity, specificity, and kinetics of the reaction. We found that peripheral blood lymphocytes from three cows with persistent lymphocytosis had 5000 to 6600 specific glucocorticoid-binding sites/cell. Compared with that reported for human lymphoid cells, glucocorticoid receptors in the bovine lymphocytes were found to have a greater affinity for the steroid with an association rate that was three times faster and a dissociation rate that was less than one-half of the former. We examined the biological half-life of hydrocortisone in the normal cow and found it to be 69.3 min, which is shorter than that reported for other domestic species and humans. The kinetics and affinity of the steroid binding may explain why in vivo glucocorticoid sensitivity was demonstrated in these animals despite the fact that elevated levels of plasma corticoids were not maintained. These results suggest that glucocorticoid sensitivity may be influenced by the nature of the binding reaction between steroid and receptor.

Psychosocial outcomes of cancer: a comparative analysis of Hodgkin's disease and testicular cancer.

PURPOSE: The psychosocial outcomes of testicular cancer and Hodgkin's disease were compared to test our hypotheses that more specific dysfunction and less hiding of symptoms would be found in the former group, as cancer visibly affects a sexual organ. Since those with Hodgkin's disease could more easily deny the disease, poorer psychosocial adjustment was predicted. PATIENTS AND METHODS: The sample consists of 85 men with Hodgkin's disease and 88 men with testicular cancer (seminomatous, n = 39; or nonseminomatous, n = 49). They were interviewed once, at least 1 year following the end of treatment. Measures of sociodemographic characteristics, physical functioning, psychologic distress, and social outcomes were collected. Treatment data were collected from medical records. RESULTS: Men with testicular cancer report more focused symptoms: less sexual enjoyment and poor health habits. Men with Hodgkin's disease report more generalized symptoms: fatigue, energy loss, and work impairment. Multivariate analysis indicates that most of these differences are site-related; independent effects of treatment on outcomes were found for more generalized symptoms. Contrary to expectations, both groups reported similar levels of infertility and erectile dysfunction. CONCLUSION: The response to testicular cancer is site-specific, while the response to Hodgkin's disease is related to both site and treatment (stage-related).

Psychosocial problems among survivors of Hodgkin's disease.

The psychosocial problems that develop in long-term survivors of Hodgkin's disease were examined in a cross-sectional survey of 403 patients. The average age at treatment was 27 years and at interview was 36 years. The median time since treatment was 9 years. Sixty percent of the patients were treated for stage I or II disease and 40% for stage III or IV. Eighty-two percent of the patients had never relapsed, and 98% were free of disease at the time of interview. The study investigated the type and frequency of problems by means of a self-administered questionnaire using standard survey items to assess disruption in three areas of life: sense of well-being, family relationships, and employment. Results indicate that energy had not returned to patients' satisfaction in 37% of the cases. This was influenced by age, time since therapy, stage of disease, and type of treatment. Patients with self-reported energy loss were more likely to be depressed. Moderately high divorce rates (32%), problems with infertility (18%), and less interest in sexual activity (20%) were reported. Employment patterns favored men returning to work, and number of hours worked was highly correlated with less depression, younger age, and return of energy. Difficulties at work were reported by 42% of the cases. The interaction of treatment, biologic, psychosocial, and functional variables is described.

Group support for patients with metastatic cancer. A randomized outcome study.

The effects of weekly supportive group meetings for women with metastatic carcinoma of the breast were systematically evaluated in a one-year, randomized, prospective outcome study. The groups focused on the problems of terminal illness, including improving relationships with family, friends, and physicians and living as fully as possible in the face of death. We hypothesized that this invention would lead to improved mood, coping strategies, and self-esteem among those in the treatment group. Eighty-six patients were tested at four-month intervals. The treatment group had significantly lower mood-disturbance scores on the Profile of Mood States scale, had fewer maladaptive coping responses, and were less phobic than the control group. This study provides objective evidence that a supportive group intervention for patients with metastatic cancer results in psychological benefit. Mechanisms underlying the effectiveness of this group intervention are explored.

Intrachain disulfide bond in the core hinge region of human IgG4.

IgG is a tetrameric protein composed of two copies each of the light and heavy chains. The four-chain structure is maintained by strong noncovalent interactions between the amino-terminal half of pairs of heavy-light chains and between the carboxyl-terminal regions of the two heavy chains. In addition, interchain disulfide bonds link each heavy-light chain and also link the paired heavy chains. An engineered human IgG4 specific for human tumor necrosis factor-alpha (CDP571) is similar to human myeloma IgG4 in that it is secreted as both disulfide bonded tetramers (approximately 75% of the total amount of IgG) and as tetramers composed of nondisulfide bonded half-IgG4 (heavy chain disulfide bonded to light chain) molecules. However, when CDP571 was genetically engineered with a proline at residue 229 of the core hinge region rather than serine, CDP571 (S229P), or with an IgG1 rather than IgG4 hinge region, CDP571(gamma 1), only trace amounts of nondisulfide bonded half-IgG tetramers were observed. Trypsin digest reversephase HPLC peptide mapping studies of CDP571 and CDP571(gamma 1) with on-line electrospray ionization mass spectroscopy supplemented with Edman sequencing identified the chemical factor preventing inter-heavy chain disulfide bond formation between half-IgG molecules: the two cysteines in the IgG4 and IgG1 core hinge region (CPSCP and CPPCP, respectively) are capable of forming an intrachain disulfide bond. Conformational modeling studies on cyclic disulfide bonded CPSCP and CPPCP peptides yielded energy ranges for the low-energy conformations of 31-33 kcal/mol and 40-42 kcal/mol, respectively. In addition, higher torsion and angle bending energies were observed for the CPPCP peptide due to backbone constraints caused by the extra proline. These modeling results suggest a reason why a larger fraction of intrachain bonds are observed in IgG4 rather than IgG1 molecules: the serine in the core hinge region of IgG4 allows more hinge region flexibility than the proline of IgG1 and thus may permit formation of a stable intrachain disulfide bond more readily.