Extended H I regions around spiral galaxies: a probe for galactic structure and the intergalactic medium
Journal Article
·
· Astrophys. J.; (United States)
The H I disks observed at large radii around nearby spiral galaxies provide sensitive probes for the mass distributions in these galaxies and of their environments. We show, for a few well-observed systems, that there is an unseen component which dominates the mass at large radii. This additional matter cannot be gas, either neutral or ionized. The data do not distinguish strongly between flat and spherical spatial distributions for this mass, though they suggest that the distribution is spherical. An observational test is proposed to differentiate the two. We investigate the thermal interaction between a hot intergalactic medium near the closure density and these extended H I regions in the assumption of magnetic field lines extended outward into the intergalactic medium (IGM). We show that, with plausible initial conditions, the intergalactic temperature at present cannot exceed 1 x 10/sup 7/ K if the H I is to have survived until now. Consideration of conditions in the past places even more stringent limits on the temperature and density of the IGM. Survival of the H I disk also implies that these galaxies cannot have persistent hot, dense halos. The X-ray observations of M31, in particular, cannot be interpreted in terms of a thermal bremsstrahlung halo model, unless this halo is younger than about 10/sup 7/ yr.
- Research Organization:
- W. K. Kellogg Radiation Laboratory, California Institute of Technology, Carnegie Institution of Washington
- OSTI ID:
- 5280980
- Journal Information:
- Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 217:3; ISSN ASJOA
- Country of Publication:
- United States
- Language:
- English
Similar Records
Hot coronas of galaxies: the effects of a dark halo, the intergalactic medium, and heat conduction
A model for the distribution of the intergalactic medium
INTERGALACTIC GAS IN GROUPS OF GALAXIES: IMPLICATIONS FOR DWARF SPHEROIDAL FORMATION AND THE MISSING BARYONS PROBLEM
Journal Article
·
Fri Jul 01 00:00:00 EDT 1988
· Astrophysics (Engl. Transl.); (United States)
·
OSTI ID:6069002
A model for the distribution of the intergalactic medium
Journal Article
·
Tue May 01 00:00:00 EDT 1990
· Astrophysical Journal; (USA)
·
OSTI ID:6709807
INTERGALACTIC GAS IN GROUPS OF GALAXIES: IMPLICATIONS FOR DWARF SPHEROIDAL FORMATION AND THE MISSING BARYONS PROBLEM
Journal Article
·
Sat Sep 10 00:00:00 EDT 2011
· Astrophysical Journal
·
OSTI ID:21584887
Related Subjects
640105* -- Astrophysics & Cosmology-- Galaxies
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COSMIC GASES
COSMIC RADIATION
COSMIC RADIO SOURCES
ELECTROMAGNETIC RADIATION
EVAPORATION
FLUIDS
GALAXIES
GASES
H1 REGIONS
H2 REGIONS
INTERGALACTIC SPACE
IONIZATION
IONIZING RADIATIONS
MAGNETIC FIELDS
PHASE TRANSFORMATIONS
RADIATIONS
SPACE
X RADIATION
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COSMIC GASES
COSMIC RADIATION
COSMIC RADIO SOURCES
ELECTROMAGNETIC RADIATION
EVAPORATION
FLUIDS
GALAXIES
GASES
H1 REGIONS
H2 REGIONS
INTERGALACTIC SPACE
IONIZATION
IONIZING RADIATIONS
MAGNETIC FIELDS
PHASE TRANSFORMATIONS
RADIATIONS
SPACE
X RADIATION