Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974a%26a....36..365s&link_type=abstract
Astronomy and Astrophysics, vol. 36, no. 3, Dec. 1974, p. 365-368.
Astronomy and Astrophysics
Astronomy
19
Astronomical Models, Galactic Nuclei, Hydrogen Clouds, Radio Astronomy, Velocity Distribution, Astronomical Maps, Hydrogen Ions, Intergalactic Media, Ionized Gases, Mass Transfer, Microwave Emission
Scientific paper
Twenty-one centimeter line observations of a high velocity H I cloud near l = +8 deg, b = -4 deg are discussed and interpreted. The cloud is approximately 3 deg in extent and has a mean line-of-sight velocity of -212.8 km/sec: the velocity dispersion is 15 km/sec. Three possible interpretations are considered: that the object may be a nearby external galaxy, that it may be an infalling high velocity H I cloud, or that it may be a cloud which has been ejected from the galactic nucleus. Of these three, the last appears most plausible on account of the close agreement with predictions based upon previously proposed models of gas ejection from the galactic nucleus.
Saraber J. M. M.
Shane William Whitney
No associations
LandOfFree
A high velocity H I cloud near the galactic center does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A high velocity H I cloud near the galactic center, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A high velocity H I cloud near the galactic center will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1336919