Results 1 to 10 of about 508,508 (133)
Neurosurgery Clinics of North America, 1999 Comatose patients are unresponsive to all external stimuli, noxious or otherwise. Neuro-ophthalmic techniques are paramount in the neurologic assessment of comatose patients, especially with regard to brain stem localization and diagnosis. Examination of the pupils, fundi, and corneal reflexes are all helpful; however, the ocular motility examination ...
openaire +3 more sources
Case Reports in Dermatology, 2009 Coma blisters are lesions that occur in the setting of a variety of neurological diseases. Although most commonly associated with barbiturate overdose, they can be seen in the setting of coma due to other etiologies. Blisters develop 48-72 h after the onset of unconsciousness.
Rocha, J +4 more
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SuperWASP Observations of the 2007 Outburst of Comet 17P/Holmes [PDF]
, 2010 We present wide-field imaging of the 2007 outburst of Comet 17P/Holmes obtained serendipitously by SuperWASP-North on 17 nights over a 42-night period beginning on the night (2007 October 22-23) immediately prior to the outburst.
Alan Fitzsimmons +51 more
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British Journal of Psychiatry, 2014 The Los Angeles-based hard-rock band Guns N’ Roses released Use Your Illusion albums (I and II) at the height of their fame. Their lesser known but no less monstrous song Coma , from album I, has no chorus, is more than 10 minutes long and is in five distinct parts.
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The Infrared Diameter -- Velocity Dispersion Relation for Elliptical Galaxies [PDF]
, 1995 Using single channel infrared photometry from the literature, a provisional K-band diameter--velocity dispersion relation for elliptical galaxies in the Coma and Virgo clusters is derived. The Coma cluster relation has \~1.5 times lower scatter at K than
Gregg, Michael D.
core +2 more sources
Particle reacceleration in Coma cluster: radio properties and hard X-ray emission [PDF]
, 2000 The radio spectral index map of the Coma halo shows a progressive steepening of the spectral index with increasing radius. Such a steepening cannot be simply justified by models involving continuous injection of fresh particles in the Coma halo or by ...
Brunetti, G. +3 more
core +2 more sources
A dozen new galaxies caught in the act: Gas stripping and extended emission line regions in the Coma cluster [PDF]
, 2010 We present images of extended H-alpha clouds associated with 14 member galaxies in the Coma cluster obtained from deep narrow band imaging observations with Suprime-Cam at the Subaru Telescope.
Abazajian +44 more
core +4 more sources
Deep UV Luminosity Functions at the Infall Region of the Coma Cluster [PDF]
, 2011 We have used deep GALEX observations at the infall region of the Coma cluster to measure the faintest UV luminosity functions (LFs) presented for a rich galaxy cluster thus far. The Coma UV LFs are measured to M_UV = -10.5 in the GALEX FUV and NUV bands,
Ferguson, H. +7 more
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Chandra X-ray Observations of Galaxies in an Off-Center Region of the Coma Cluster
, 2005 We have performed a pilot Chandra survey of an off-center region of the Coma cluster to explore the X-ray properties and Luminosity Function of normal galaxies.
Alexander, D. M. +6 more
core +1 more source
Solar-insolation-induced changes in the coma morphology of comet 67P/Churyumov-Gerasimenko. Optical monitoring with the Nordic Optical Telescope [PDF]
, 2017 Context. 67P/Churyumov-Gerasimenko (67P/C-G) is a short-period Jupiter family comet with an orbital period of 6.55 years. Being the target comet of ESA’s Rosetta mission, 67P/C-G has become one of the most intensively studied minor bodies of the Solar ...
A. Somero +21 more
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