TY - JOUR
T1 - THE PROPERTIES of the CIRCUMGALACTIC MEDIUM in RED and BLUE GALAXIES
T2 - RESULTS from the COS-GASS+COS-HALOS SURVEYS
AU - Borthakur, Sanchayeeta
AU - Heckman, Timothy
AU - Tumlinson, Jason
AU - Bordoloi, Rongmon
AU - Kauffmann, Guinevere
AU - Catinella, Barbara
AU - Schiminovich, David
AU - Davé, Romeel
AU - Moran, Sean M.
AU - Saintonge, Amelie
N1 - Publisher Copyright:
© 2016 Published by Elsevier B.V.
PY - 2016/12/20
Y1 - 2016/12/20
N2 - We use the combined data from the COS-GASS and COS-Halos surveys to characterize the Circum-Galactic Medium (CGM) surrounding typical low-redshift galaxies in the mass range M∗ ∼ 109.5-11.5 Ṁ, and over a range of impact parameters extending to just beyond the halo virial radius (Rvir). We find the radial scale length of the distributions of the equivalent widths of the Lyα and Si III absorbers to be ∼1 and ∼ 0.4 Rvir, respectively. The radial distribution of equivalent widths is relatively uniform for the blue galaxies, but highly patchy (i.e., it has a low covering fraction) for the red galaxies. We also find that the Lyαand Si III equivalent widths show significant positive correlations with the specific star formation rate (sSFR) of the galaxy. We find a surprising lack of correlations between the halo mass (virial velocity) and either the velocity dispersions or velocity offsets of the Lyαlines. The ratio of the velocity offset to the velocity dispersion for the Lyαabsorbers has a mean value of ∼4, suggesting that a given line of sight is intersecting a dynamically coherent structure in the CGM, rather than a sea of orbiting clouds. The kinematic properties of the CGM are similar in the blue and red galaxies, although we find that a significantly larger fraction of the blue galaxies have large Lyαvelocity offsets (>200 km s-1). We show that-if the CGM clouds represent future fuel for star formation-our new results could imply a large drop in the sSFR across the galaxy mass-range we probe.
AB - We use the combined data from the COS-GASS and COS-Halos surveys to characterize the Circum-Galactic Medium (CGM) surrounding typical low-redshift galaxies in the mass range M∗ ∼ 109.5-11.5 Ṁ, and over a range of impact parameters extending to just beyond the halo virial radius (Rvir). We find the radial scale length of the distributions of the equivalent widths of the Lyα and Si III absorbers to be ∼1 and ∼ 0.4 Rvir, respectively. The radial distribution of equivalent widths is relatively uniform for the blue galaxies, but highly patchy (i.e., it has a low covering fraction) for the red galaxies. We also find that the Lyαand Si III equivalent widths show significant positive correlations with the specific star formation rate (sSFR) of the galaxy. We find a surprising lack of correlations between the halo mass (virial velocity) and either the velocity dispersions or velocity offsets of the Lyαlines. The ratio of the velocity offset to the velocity dispersion for the Lyαabsorbers has a mean value of ∼4, suggesting that a given line of sight is intersecting a dynamically coherent structure in the CGM, rather than a sea of orbiting clouds. The kinematic properties of the CGM are similar in the blue and red galaxies, although we find that a significantly larger fraction of the blue galaxies have large Lyαvelocity offsets (>200 km s-1). We show that-if the CGM clouds represent future fuel for star formation-our new results could imply a large drop in the sSFR across the galaxy mass-range we probe.
KW - galaxies: halos
KW - galaxies: star formation
KW - quasars: absorption lines
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U2 - 10.3847/1538-4357/833/2/259
DO - 10.3847/1538-4357/833/2/259
M3 - Article
AN - SCOPUS:85007545445
SN - 0004-637X
VL - 833
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 259
ER -