21-cm H I emission from the Damped Lyman-alpha absorber SBS 1543+593
arXiv:astro-ph/0104396 · doi:10.1051/0004-6361:20010592
Abstract
We detect 21-cm emission from the Low Surface Brightness (LSB) galaxy SBS 1543+593, which gives rise to a Damped Lyman-alpha (DLA) absorption line in the spectrum of the background QSO HS 1543+5921 (z=0.807). We obtain an accurate measure of the velocity of the H I gas in the LSB galaxy, v=2868 km/s, and derive a mass of 1.3e9 solar masses. We compare this value with limits obtained towards two other z~0.1 DLA systems, and show that SBS 1543+593 would not have been detected. Hence LSB galaxies similar to SBS 1543+593 can be responsible for DLA systems at even modest redshifts without being detectable from their 21-cm emission.
4 pages, 1 figure, accepted for publication in A&A
References in corpus (2)
Cited by in corpus (15)
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