The corona contracts in a black-hole transient.

The geometry of the accretion flow around stellar-mass black holes can change on timescales of days to months1-3. When a black hole emerges from quiescence (that is, it 'turns on' after accreting material from its companion) it has a very hard (high-energy) X-ray spectrum produced by a hot corona4,5 positioned above its accretion disk, and then transitions to a soft (lower-energy) spectrum dominated by emission from the geometrically thin accretion disk, which extends to the innermost stable circular orbit6,7. Much debate persists over how this transition occurs and whether it is driven largely by a reduction in the truncation radius of the disk8,9 or by a reduction in the spatial extent of the corona10,11. Observations of X-ray reverberation lags in supermassive black-hole systems12,13 suggest that the corona is compact and that the disk extends nearly to the central black hole14,15. Observations of stellar-mass black holes, however, reveal equivalent (mass-scaled) reverberation lags that are much larger16, leading to the suggestion that the accretion disk in the hard-X-ray state of stellar-mass black holes is truncated at a few hundreds of gravitational radii from the black hole17,18. Here we report X-ray observations of the black-hole transient MAXI J1820+07019,20. We find that the reverberation time lags between the continuum-emitting corona and the irradiated accretion disk are 6 to 20 times shorter than previously seen. The timescale of the reverberation lags shortens by an order of magnitude over a period of weeks, whereas the shape of the broadened iron K emission line remains remarkably constant. This suggests a reduction in the spatial extent of the corona, rather than a change in the inner edge of the accretion disk.

The recent expansion of Pluto's atmosphere.

Stellar occultations--the passing of a relatively nearby body in front of a background star--can be used to probe the atmosphere of the closer body with a spatial resolution of a few kilometres (ref. 1). Such observations can yield the scale height, temperature profile, and other information about the structure of the occulting atmosphere. Occultation data acquired for Pluto's atmosphere in 1988 revealed a nearly isothermal atmosphere above a radius of approximately 1,215 km. Below this level, the data could be interpreted as indicating either an extinction layer or the onset of a large thermal gradient, calling into question the fundamental structure of this atmosphere. Another question is to what extent Pluto's atmosphere might be collapsing as it recedes from the Sun (passing perihelion in 1989 in its 248-year orbital period), owing to the extreme sensitivity of the equilibrium surface pressure to the surface temperature. Here we report observations at a variety of visible and infrared wavelengths of an occultation of a star by Pluto in August 2002. These data reveal evidence for extinction in Pluto's atmosphere and show that it has indeed changed, having expanded rather than collapsed, since 1988.

Virtual glioblastoma: growth, migration and treatment in a three-dimensional mathematical model.

OBJECTIVES: Glioblastomas are aggressive primary brain cancers that are characterized by extensive infiltration into the brain and are highly resistant to treatment. Through mathematical modelling, we model the process of invasion and predict the relative importance of mechanisms contributing to malignant invasion. Clinically, we predict patterns of tumour recurrence following various modes of therapeutic intervention. MATERIALS AND METHODS: Our mathematical model uses a realistic three-dimensional brain geometry and considers migrating and proliferating cells as separate classes. Several mechanisms for infiltrative migration are considered. Methods are developed for simulating surgical resection, radiotherapy and chemotherapy. RESULTS: The model provides clinically realistic predictions of tumour growth and recurrence following therapeutic intervention. Specific results include (i) invasiveness is governed largely by the ability of glioblastoma cells to degrade and migrate through the extracellular matrix and the ability of single migrating cells to form colonies; (ii) tumours originating deeper in the brain generally grow more quickly than those of superficial origin; (iii) upon surgery, the margins and geometry of resection significantly determine the extent and pattern of postoperative recurrence; (iv) radiotherapy works synergistically with greater resection margins to reduce recurrence; (v) simulations in both two- and three-dimensional geometries give qualitatively similar results; and (vi) in an actual clinical case comprising several surgical interventions, the model provides good qualitative agreement between the simulated and observed course of the disease. CONCLUSIONS: The model provides a useful initial framework by which biological mechanisms of invasion and efficacy of potential treatment regimens may be assessed.

Chronic muscle pain induced by repeated acid Injection is reversed by spinally administered mu- and delta-, but not kappa-, opioid receptor agonists.

Opioids are commonly used for pain relief clinically and reduce hyperalgesia in most animal models. Two injections of acidic saline into one gastrocnemius muscle 5 days apart produce a long-lasting bilateral hyperalgesia without associated tissue damage. The current study was undertaken to assess the effects of opioid agonists on mechanical hyperalgesia induced by repeated intramuscular injections of acid. Morphine (mu-agonist), [D-Ala(2),N-Me-Phe(4),Gly-ol(5)]-enkephalin (mu-agonist; DAMGO), 4-[((alpha)R)-alpha-((2S,5R)-4-allyl-2,5-dimethyl-1-piperazinyl)-3-methoxybenzyl]-N,N-diethylbenzamide (delta-agonist; SNC80), or (1S-trans)-3,4-dichloro-N-methyl-N-[2-(1-pyrrolidinyl)cylcohexyl]-benzeneacetamide hydrochloride (kappa-agonist; U50,488) were administered intrathecally to activate opioid receptors once hyperalgesia was developed. Mechanical hyperalgesia was assessed by measuring the withdrawal thresholds to mechanical stimuli (von Frey filaments) before the first and second intramuscular injection, 24 h after the second intramuscular injection, and for 1 h after administration of the opioid agonist or vehicle. Morphine, DAMGO, and SNC80 dose dependently increased the mechanical withdrawal threshold back toward baseline responses. The reduction in hyperalgesia produced by morphine and DAMGO was prevented by H-D-Phe-Cys-Tyr-D-Trp-Arg-Thr-Pen-Thr-NH(2) (CTAP) and that of SNC80 was prevented by naltrindole. U50,488 had no effect on the decreased mechanical withdrawal thresholds. Thus, activation of mu- and delta-, but not kappa-, opioid receptors in the spinal cord reduces mechanical hyperalgesia following repeated intramuscular injection of acid, thus validating the use of this new model of chronic muscle pain.