2004/09/13 by K. S. Dwarakanath, Dwarakanath, K. S.
Physics and Astronomy · #Astrophysics (astro-ph) #Astrophysics and Star Formation Studies #FOS: Physical sciences #Radio Astronomy Observations and Technology #Superconducting and THz Device Technology #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0409277
5 pages, 6 figures, uses basi.cls, to be published in Bull. Astr. Soc. India
arxiv created 2004/09/13 · openalex publication_date 2004/09/13 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
A high latitude HI 21 cm-line absorption survey toward extragalactic sources was recently completed using the Giant Meterwave Radio Telescope (GMRT). A total of 104 sources with mod(b) > 15 deg. and with a 21 cm flux density greater than 1 Jy were observed for about 120 hours. With an optical depth detection limit of about 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 about 7.6 km/s. 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 about 21 km/s. About 20 percent of the total number 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.