Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/734
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dc.contributor.authorDwarakanath, K. S-
dc.date.accessioned2006-03-13T09:52:20Z-
dc.date.available2006-03-13T09:52:20Z-
dc.date.issued2004-09-
dc.identifier.citationBASI, Vol. 32, No. 3, pp. 215-221en
dc.identifier.urihttp://hdl.handle.net/2248/734-
dc.description.abstracthigh 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 Banken
dc.format.extent137115 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectISM: cloudsen
dc.subjectkinematics and dynamics Radio linesen
dc.subjectISMen
dc.titleKinematics of diffuse interstellar clouds: recent GMRT resultsen
dc.typeArticleen
Appears in Collections:BASI Publications

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