dc.contributor.author |
Dwarakanath, K. S |
|
dc.date.accessioned |
2006-03-13T09:52:20Z |
|
dc.date.available |
2006-03-13T09:52:20Z |
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dc.date.issued |
2004-09 |
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dc.identifier.citation |
BASI, Vol. 32, No. 3, pp. 215-221 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/734 |
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dc.description.abstract |
high latitude HI 21 cm-line absorption survey towards extragalactic sources was recently completed using the Giant Meterwave Radio Telescope (GMRT). A total of 104 sources with |b|>15o and with a 21 cm ¤ux density greater than 1 Jy were observed for ~120 hours. With an optical depth detection limit of ~ 0.01 this is the most sensitive high-latitude survey as yet. Most of the detected HI 21 cm-line absorption features belong to a population with a velocity dispersion of ~7.6 km s-1. These are the standard HI clouds and have been well-studied for decades. However, we also detect a second population of absorbing clouds with a velocity dispersion of ~ 21 km s-1. About 20% of the total population of absorbing clouds belong to this population. This new population of fast clouds can be identified with a similar velocity dispersion Ca II absorbing clouds and with the Halo clouds recently detected in HI emission from Green Bank |
en |
dc.format.extent |
137115 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.subject |
ISM: clouds |
en |
dc.subject |
kinematics and dynamics Radio lines |
en |
dc.subject |
ISM |
en |
dc.title |
Kinematics of diffuse interstellar clouds: recent GMRT results |
en |
dc.type |
Article |
en |