… Ae Pre-Main-Sequence Stars and from Debris Disks around Young Stars: Warm and Cold Circumstellar … -
WF Thi, EF van Dishoeck, GA Blake, GJ van … - The Astrophysical Journal, 2001 - UChicago Press
... The warm gas is typically 1%?10% of the total mass deduced from millimeter continuum ...
Thus, residual molecular gas may persist into the debris-disk phase. ...
Observable Properties of X-Ray--heated Winds in Active Galactic Nuclei: Warm Reflectors and Warm … -
JH Krolik, GA Kriss - The Astrophysical Journal, 1995 - UChicago Press
... Abstract, First discovered by spectropolarimetry, the warm reflecting gas near
active galactic nuclei (AGNs) may be observed in many ways. ...
Warm gas and spatial variations of molecular excitation in the nuclear region of IC 342 -
A Eckart, D Downes, R Genzel, AI Harris, DT Jaffe, … - Astrophysical Journal, 1990 - adsabs.harvard.edu
... there may be CO emission from optically thin gas at a temperature of ?= 40 K.
Alternatively the `2CO line emission originates in a small amount of warm gas ...
Baryons in the Warm-Hot Intergalactic Medium -
R Dave, R Cen, JP Ostriker, GL Bryan, L Hernquist, … - The Astrophysical Journal, 2001 - UChicago Press
... We expect that the evolution of warm-hot gas ... by shock heating of intergalactic gas
onto large ... as resolution, volume, and hydrodynamic algorithm may also play ...
Theories of the Hot Interstellar Gas -
L Spitzer Jr - Annual Reviews in Astronomy and Astrophysics, 1990 - Annual Reviews
... about the same as those in the warm ionized medium (43), a model of straight, parallel
lines of force extending into the hot gas may, perhaps, provide a ...
Warm Absorbers in Active Galactic Nuclei: A Multitemperature Wind -
JH Krolik, GA Kriss - The Astrophysical Journal, 2001 - UChicago Press
... For this reason, many photoionization models of warm absorbers have ... 2001), suggesting
that there may be substantial amounts of gas with ? 100 ...
Warm gas in central regions of nearby galaxies -
M Dumke, C Nieten, G Thuma, R Wielebinski, W Walsh - A&A, 2001 - aanda.org
... therefore only excited if the gas is sufficiently warm and/or ... immediate surroundings
of star forming regions, where gas properties may be different. ...
Where Are the Baryons? -
R Cen, JP Ostriker - The Astrophysical Journal, 1999 - UChicago Press
... ray clusters owing to the warm/hot component, as seen in Figure 3. Fifth, the
warm/hot gas may show up as very broad, relatively weak (mostly having cm -2 ...
The clinical impact of warmed insufflation carbon dioxide gas for laparoscopic cholecystectomy -
S Saad - Surgical Endoscopy, 2000 - Springer
... did not find a significant difference between cold gas and warm gas in- sufflation
in rectal temperature changes. These oberserva- tions may be explained by ...
Thermal phases of interstellar and quasar gas -
S Lepp, R McCray, JM Shull, DT Woods, T Kallman - Astrophysical Journal, 1985 - UChicago Press
... 100,000 K); warm gas (T about 10,000 K); and cold gas (T less than 100 K). With
attenuation of ultraviolet and X-ray radiation, the cold phase may undergo a ...
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