A Green Bank Telescope Survey for H I 21 cm Absorption in the Disks and Halos of Low Red-Shifts Galaxies*
This is the pre-published version harvested from ArXiv. The published version is located at http://iopscience.iop.org/0004-637X/727/1/52/
We present an H I 21 cm absorption survey with the Green Bank Telescope (GBT) of galaxy-quasar pairs selected by combining galaxy data from the Sloan Digital Sky Survey (SDSS) and radio sources from the Faint Images of the Radio Sky at Twenty-Centimeters (FIRST) survey. Our sample consists of 23 sight lines through 15 low-redshift foreground galaxy-background quasar pairs with impact parameters ranging from 1.7 kpc up to 86.7 kpc. We detected one absorber in the GBT survey from the foreground dwarf galaxy, GQ1042+0747, at an impact parameter of 1.7 kpc and another possible absorber in our follow-up Very Large Array (VLA) imaging of the nearby foreground galaxy UGC 7408. The line widths of both absorbers are narrow (FWHM of 3.6 and 4.8km s–1). The absorbers have sub-damped Lyα column densities, and most likely originate in the disk gas of the foreground galaxies. We also detected H I emission from three foreground galaxies including UGC 7408. Although our sample contains both blue and red galaxies, the two H I absorbers as well as the H I emissions are associated with blue galaxies. We discuss the physical conditions in the 21 cm absorbers and some drawbacks of the large GBT beam for this type of survey.
S Borthakur, TM Tripp, Min Yun, DV Bowen, JD Meiring, DG York, and E Momjian. "A Green Bank Telescope Survey for H I 21 cm Absorption in the Disks and Halos of Low Red-Shifts Galaxies*" Astronomical Journal 727.1 (2011): 52-52.
Available at: http://works.bepress.com/min_yun/17