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http://hdl.handle.net/2248/734
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DC Field | Value | Language |
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dc.contributor.author | Dwarakanath, K. S | - |
dc.date.accessioned | 2006-03-13T09:52:20Z | - |
dc.date.available | 2006-03-13T09:52:20Z | - |
dc.date.issued | 2004-09 | - |
dc.identifier.citation | BASI, Vol. 32, No. 3, pp. 215-221 | en |
dc.identifier.uri | http://hdl.handle.net/2248/734 | - |
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 | - |
dc.format.mimetype | application/pdf | - |
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 |
Appears in Collections: | BASI Publications |
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File | Description | Size | Format | |
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0432215.PDF | 133.9 kB | Adobe PDF | View/Open |
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