Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger.

The merger of two neutron stars is predicted to give rise to three major detectable phenomena: a short burst of γ-rays, a gravitational-wave signal, and a transient optical-near-infrared source powered by the synthesis of large amounts of very heavy elements via rapid neutron capture (the r-process). Such transients, named 'macronovae' or 'kilonovae', are believed to be centres of production of rare elements such as gold and platinum. The most compelling evidence so far for a kilonova was a very faint near-infrared rebrightening in the afterglow of a short γ-ray burst at redshift z = 0.356, although findings indicating bluer events have been reported. Here we report the spectral identification and describe the physical properties of a bright kilonova associated with the gravitational-wave source GW170817 and γ-ray burst GRB 170817A associated with a galaxy at a distance of 40 megaparsecs from Earth. Using a series of spectra from ground-based observatories covering the wavelength range from the ultraviolet to the near-infrared, we find that the kilonova is characterized by rapidly expanding ejecta with spectral features similar to those predicted by current models. The ejecta is optically thick early on, with a velocity of about 0.2 times light speed, and reaches a radius of about 50 astronomical units in only 1.5 days. As the ejecta expands, broad absorption-like lines appear on the spectral continuum, indicating atomic species produced by nucleosynthesis that occurs in the post-merger fast-moving dynamical ejecta and in two slower (0.05 times light speed) wind regions. Comparison with spectral models suggests that the merger ejected 0.03 to 0.05 solar masses of material, including high-opacity lanthanides.

The unusual gamma-ray burst GRB 101225A explained as a minor body falling onto a neutron star.

The tidal disruption of a solar-mass star around a supermassive black hole has been extensively studied analytically and numerically. In these events, the star develops into an elongated banana-shaped structure. After completing an eccentric orbit, the bound debris falls into the black hole, forming an accretion disk and emitting radiation. The same process may occur on planetary scales if a minor body passes too close to its star. In the Solar System, comets fall directly into our Sun or onto planets. If the star is a compact object, the minor body can become tidally disrupted. Indeed, one of the first mechanisms invoked to produce strong gamma-ray emission involved accretion of comets onto neutron stars in our Galaxy. Here we report that the peculiarities of the 'Christmas' gamma-ray burst (GRB 101225A) can be explained by a tidal disruption event of a minor body around an isolated Galactic neutron star. This would indicate either that minor bodies can be captured by compact stellar remnants more frequently than occurs in the Solar System or that minor-body formation is relatively easy around millisecond radio pulsars. A peculiar supernova associated with a gamma-ray burst provides an alternative explanation.

GRB 090423 at a redshift of z approximately 8.1.

Gamma-ray bursts (GRBs) are produced by rare types of massive stellar explosion. Their rapidly fading afterglows are often bright enough at optical wavelengths that they are detectable at cosmological distances. Hitherto, the highest known redshift for a GRB was z = 6.7 (ref. 1), for GRB 080913, and for a galaxy was z = 6.96 (ref. 2). Here we report observations of GRB 090423 and the near-infrared spectroscopic measurement of its redshift, z = 8.1(-0.3)(+0.1). This burst happened when the Universe was only about 4 per cent of its current age. Its properties are similar to those of GRBs observed at low/intermediate redshifts, suggesting that the mechanisms and progenitors that gave rise to this burst about 600,000,000 years after the Big Bang are not markedly different from those producing GRBs about 10,000,000,000 years later.

An optical supernova associated with the X-ray flash XRF 060218.

Long-duration gamma-ray bursts (GRBs) are associated with type Ic supernovae that are more luminous than average and that eject material at very high velocities. Less-luminous supernovae were not hitherto known to be associated with GRBs, and therefore GRB-supernovae were thought to be rare events. Whether X-ray flashes--analogues of GRBs, but with lower luminosities and fewer gamma-rays--can also be associated with supernovae, and whether they are intrinsically 'weak' events or typical GRBs viewed off the axis of the burst, is unclear. Here we report the optical discovery and follow-up observations of the type Ic supernova SN 2006aj associated with X-ray flash XRF 060218. Supernova 2006aj is intrinsically less luminous than the GRB-supernovae, but more luminous than many supernovae not accompanied by a GRB. The ejecta velocities derived from our spectra are intermediate between these two groups, which is consistent with the weakness of both the GRB output and the supernova radio flux. Our data, combined with radio and X-ray observations, suggest that XRF 060218 is an intrinsically weak and soft event, rather than a classical GRB observed off-axis. This extends the GRB-supernova connection to X-ray flashes and fainter supernovae, implying a common origin. Events such as XRF 060218 are probably more numerous than GRB-supernovae.

A framework for risk assessment and decision-making strategies in dangerous good transportation.

The risk from dangerous goods transport by road and strategies for selecting road load/routes are faced in this paper, by developing an original site-oriented framework of general applicability at local level. A realistic evaluation of the frequency must take into account on one side inherent factors (e.g. tunnels, rail bridges, bend radii, slope, characteristics of neighborhood, etc.) on the other side factors correlated to the traffic conditions (e.g. dangerous goods trucks, etc.). Field data were collected on the selected highway, by systematic investigation, providing input data for a database reporting tendencies and intrinsic parameter/site-oriented statistics. The developed technique was applied to a pilot area, considering both the individual risk and societal risk and making reference to flammable and explosive scenarios. In this way, a risk assessment, sensitive to route features and population exposed, is proposed, so that the overall uncertainties in risk analysis can be lowered.

Evaluation of diffusional resistances in the process of glucose isomerization to fructose by immobilized glucose isomerase.

A kinetic model presented in a previous work is employed to carry out a systematic study dealing with the relative importance of intraparticle and interparticle diffusional resistances in the process of glucose isomerization to fructose by immobilized glucose isomerase. An analytical generalized expression of the effectiveness factor is obtained, which promises to be particularly useful for design purposes. Finally, the role of each of the main parameters influencing the catalyst effectiveness factor is put in evidence and discussed within the whole range of possible operative conditions.

Discovery of a transient absorption edge in the X-ray spectrum of GRB 990705.

We report the discovery of a transient equivalent hydrogen column density with an absorption edge at approximately 3.8 kiloelectron volts in the spectrum of the prompt x-ray emission of gamma-ray burst (GRB) 990705. This feature can be satisfactorily modeled with a photoelectric absorption by a medium located at a redshift of approximately 0.86 and with an iron abundance of approximately 75 times the solar one. The transient behavior is attributed to the strong ionization produced in the circumburst medium by the GRB photons. The high iron abundance points to the existence of a burst environment enriched by a supernova along the line of sight. The supernova explosion is estimated to have occurred about 10 years before the burst. Our results agree with models in which GRBs originate from the collapse of very massive stars and are preceded by a supernova event.

Generalized linearization of kinetics of glucose isomerization to fructose by immobilized glucose isomerase.

The kinetic parameters of both glucose isomerization to fructose and immobilized glucose isomerase (GI) inactivation calculated under different conditions are compared and discussed. Utilizing these figures, the possibility of generalizing a linear model, previously proposed for the kinetics of glucose isomerization by immobilized glucose isomerase, is investigated, so as to apply them to whole ranges of temperature and concentrations of actual interest in industrial processes. The proposed model is a satisfactory approximation of the more involved Briggs-Haldane approach and substantially simplifies the problem of optimizing an industrial fixed-bed column for high-fructose corn syrup (HFCS) production.

Decay of the GRB 990123 optical afterglow: implications for the fireball model

Broad-band (ultraviolet to near-infrared) observations of the intense gamma ray burst GRB 990123 started approximately 8.5 hours after the event and continued until 18 February 1999. When combined with other data, in particular from the Robotic Telescope and Transient Source Experiment (ROTSE) and the Hubble Space Telescope (HST), evidence emerges for a smoothly declining light curve, suggesting some color dependence that could be related to a cooling break passing the ultraviolet-optical band at about 1 day after the high-energy event. The steeper decline rate seen after 1.5 to 2 days may be evidence for a collimated jet pointing toward the observer.

Photometry and spectroscopy of the GRB 970508 optical counterpart

An optical transient within the error box of the gamma ray burst GRB 970508 was imaged 4 hours after the event. It displayed a strong ultraviolet excess, and reached maximum brightness 2 days later. The optical spectra did not show any emission lines, and no variations on time scales of minutes were observed for 1 hour during the decline phase. According to the fireball and afterglow models, the intensity should rise monotonically before the observed optical maximum, but the data indicate that another physical mechanism may be responsible for the constant phase seen during the first hours after the burst.

Biochemical evidence of functional interaction between mu- and delta-opioid receptors in SK-N-BE neuroblastoma cell line.

Radioligand binding assays and functional experiments revealed that the SK-N-BE neuroblastoma cell line expresses a similar ratio of mu- and delta-opioid receptors, both negatively coupled to adenylyl cyclase through pertussis toxin-sensitive G proteins. Our findings also indicate that some functional interaction occurred between the two opioid subtypes; in fact, long-term exposure to [D-Ala2-N-methyl-Phe4-Gly-ol5]enkephalin (DAMGO), a mu-selective agonist, sensitized the functional response of the delta-selective agonist but not vice versa. It is interesting that in acute interaction experiments, we observed a shift to the right of the concentration-effect curve of either DAMGO or [D-Pen2,5]enkephalin (DPDPE), a delta-selective agonist, as a result of DPDPE or DAMGO administration, respectively. In addition, low doses of naloxone, an antagonist selective for mu receptors, increased the inhibitory effect [D-Ala2-D-Met5]enkephalinamide (DAME), a mixed mu/delta agonist, on adenylyl cyclase activity. Taken overall, these data support the hypothesis of the existence of a cross talk between mu and delta receptors in the SK-N-BE cell line.

5-HT1D receptor type is involved in stimulation of cell proliferation by serotonin in human small cell lung carcinoma.

Serotonin (5-hydroxytryptamine, 5-HT), a neurotransmitter and vasoactive agent, is contained in two small cell lung carcinoma cell lines GLC8 and NCI-N-592 and is released in the culture medium. It also stimulates DNA synthesis in the same cell lines. In GLC8 cells this mitogenic effect is not counteracted by ketanserin, ICS 205-930 and GR 113-808 which are antagonists of the 5-HT2, 5-HT3 and 5-HT4 receptors, respectively. On the contrary, the antagonists metergoline, methysergide, SDZ 21-009 and methiothepin inhibit the 5-HT-stimulated incorporation of [3H]thymidine in GLC8 cells. The 5-HT1D agonist sumatriptan is capable of mimicking 5-HT action on cell proliferation. Both sumatriptan and 5-HT inhibit adenylate cyclase activity at doses which correlate with the mitogenic effect. We conclude that a 5-HT1D receptor type contributes to the mitogenic effect of 5-HT in GLC8 cells. This is the first demonstration of an involvement of the 5-HT1D receptor type in human cell proliferation. The design of specific antagonists for this type of receptor might be useful for the growth control of this very aggressive tumor.

Galanin reduces carbachol stimulation of phosphoinositide turnover in rat ventral hippocampus by lowering Ca2+ influx through voltage-sensitive Ca2+ channels.

The 29-amino-acid peptide galanin (GAL) caused concentration-dependent inhibition of the accumulation of 3H-inositol phosphates (3H-InsPs) induced by the muscarinic agonist carbachol (CARB; 10(-3)-10(-5) M) in the presence of 5 mM lithium, specifically in tissue miniprisms from rat ventral hippocampus. The inhibitory effect of GAL involved the mono-, bis-, tris-, and tetrakisphosphates formed during activation for 2 min of phospholipase C by CARB (1 mM) in the absence of lithium. GAL (1 microM) did not affect alpha-adrenergic or serotonergic type 2 receptor-mediated phosphoinositide (PI) breakdown in the same tissue. GAL by itself neither acted on basal levels of 3H-InsPs nor affected muscarinic receptors in binding studies. Blockade of the T-, N-, and L-types of voltage-sensitive calcium channel (VSCC) with 200 microM Cd2+ reduced muscarinic receptor-mediated PI breakdown by 50% and abolished the inhibitory effect of GAL (1 microM). Reduction of the extracellular Ca2+ concentration from 1.3 mM to 0.49 microM abolished the GAL inhibition of CARB-stimulated PI hydrolysis. Ca2+ influx promoted by 18 mM K+ depolarization or by 1 microM Bay K 8644, a selective agonist of the L-type VSCC, prevented the inhibitory effect of GAL. Blockade of the L-type VSCC with nifedipine (1 microM) potentiated the inhibitory effects of GAL without affecting muscarinic stimulation of PI breakdown.(ABSTRACT TRUNCATED AT 250 WORDS)

Mode of action of tiaspirone on the central cholinergic system.

Tiaspirone, a potential antipsychotic drug, reduced the acetylcholine content of rat hemispheric brain regions (striatum 35%, hippocampus 20%, cortex 32% with no effect on N. accumbens) at an oral dose of 40 mg/kg. Choline content was uniformly raised in the same brain regions. A kinetic study showed that the drug is evenly distributed in the brain. Tiaspirone's effects on acetylcholine and choline in the striatum were not related in time. The fall off (30-240 min) of tiaspirone's effect on choline content paralleled the decline in striatal drug concentration (t1/2 = 240 min) whereas that on acetylcholine did not. No tolerance was observed to an acute challenge with tiaspirone on acetylcholine and choline in the striatum after 11 days' subchronic treatment. In vitro the drug had no effect on striatal choline acetyltransferase and acetylcholinesterase activities up to a concentration of 300 microM. The muscarinic agonist oxotremorine did not interfere with the acetylcholine decrease produced by the drug suggesting that muscarinic receptors are not essential for this effect. Tiaspirone, however, was found to be a competitive, reversible inhibitor of the sodium-dependent high-affinity choline uptake (SDHACU) by crude hippocampal and striatal synaptosomal preparations, giving IC50 values of respectively 3.69 microM and 1.14 microM. The compound did not alter SDHACU ex vivo despite the fact that it readily crosses the blood-brain barrier and achieves brain concentrations equivalent to its in vitro IC50 concentration. Tiaspirone antagonized the striatal acetylcholine increasing effect of apomorphine, a selective dopaminergic receptor agonist, supporting the idea that the drug affects the striatal cholinergic system by a primary action on dopamine receptors.(ABSTRACT TRUNCATED AT 250 WORDS)

Enhancement of opioid cataleptic response by cortical frontal deafferentation or intrastriatal injection of NMDA-receptor antagonists.

The cataleptic activity of morphine and methadone was markedly potentiated in frontally decorticated rats with no apparent changes in the onset or duration of action. Enhancement of the opioid cataleptic response was not due to changes in the availability of the drugs in the brain. The potentiation of methadone-induced catalepsy in decorticated rats was mimicked in naive rats by intrastriatal (i.s.) application of 2-amino-7-phosphonoheptanoic acid (AP7), a potent and selective antagonist of N-methyl-D-aspartate (NMDA) receptors. Therefore, degeneration of glutamatergic synapses following decortication could be responsible for the changes in behavioral effects caused by opioids. The failure of AP7 to elicit an effect after injection into the n. accumbens fits with the possibility of a selective involvement of the striatum in this phenomenon. That the striatum plays a critical role in the expression of opioid-induced catalepsy was substantiated by the findings that: (1) naloxone, an opioid antagonist, injected i.s., prevents the potentiation of catalepsy induced by methadone and morphine in decorticated animals, (2) oxotremorine, a muscarinic agonist, injected i.s., reverses the enhancement of opioid-catalepsy in decorticated rats, (3) earlier studies by others showed that ablation of the striatum had a facilitatory action on opioid-induced catalepsy. In conclusion, evidence is given that the corticostriatal pathway exerts an inhibitory effect upon narcotic-induced cataleptic behavior. The possibility that this effect is mediated through striatonigral GABAergic output is discussed. The data further suggest that the neuronal mechanisms through which the corticostriatal pathway mediates narcotic catalepsy is operative through activation of NMDA receptors within the striatum.

Acute and chronic studies on functional aspects of coexistence.

Autoinhibition of acetylcholine release by the coexisting peptide galanin in the septal afferents to the hippocampus of the rat was examined in tissue slices from the hippocampus. Galanin inhibits the evoked release of the coexisting neurotransmitter, acetylcholine, in the ventral hippocampus, providing an example of autoinhibition of release of a neurotransmitter by one of the coexisting neurotransmitters. The galanin mediated inhibition of the acetylcholine release is a complement to the well known strong cholinergic autoinhibition. The effects of the coexisting galanin and acetylcholine on several second messenger systems were also examined: acetylcholine acting at muscarinic receptors depresses cyclic adenosine 3',5'-monophosphate and stimulates elevation of cyclic guanosine 3',5'-monophosphate levels, whereas neither cyclic adenosine 3',5'-monophosphate nor cyclic guanosine 3',5'-monophosphate levels were affected by galanin (1 microM). Galanin however inhibited partly the muscarinic stimulation of phosphoinositide breakdown, suggesting that inositol phosphate(s) or diacylglycerol may act as second messenger(s) of the galanin action in the hippocampus. The effects of chronic changes in firing rate on the coexisting neurotransmitters in the rat ventral spinal cord containing serotonin, thyrotropin releasing hormone, substance P and substance K were examined. The tissue levels of the coexisting transmitters were studied in rats chronically treated with imipramine (14 days; 2 x 10 mumoles/kg/day) and zimelidine (14 days; 2 x 10 mumoles/kg/day). Upon treatment with zimelidine the tissue levels of the serotonin metabolite 5-hydroxyindoleacetic acid fall by 32% while thyrotropin releasing hormone levels seem to increase 35% and substance P/substance K levels also increase 48 and 72% respectively. Imipramine treatment resulted in similar although less pronounced changes.(ABSTRACT TRUNCATED AT 250 WORDS)