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Kinematics of diffuse interstellar clouds: recent GMRT results

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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


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