Edinburgh Research Explorer

The Properties of the Circumgalactic Medium in Red and Blue Galaxies: Results from the COS-GASS+COS-Halos Surveys

Research output: Contribution to journalArticle

  • Sanchayeeta Borthakur
  • Timothy Heckman
  • Jason Tumlinson
  • Rongmon Bordoloi
  • Guinevere Kauffmann
  • Barbara Catinella
  • David Schiminovich
  • Romeel Davé
  • Sean M. Moran
  • Amelie Saintonge

Related Edinburgh Organisations

Open Access permissions

Open

Documents

https://arxiv.org/abs/1609.06308
Original languageEnglish
Pages (from-to)259
JournalAstrophysical Journal
Volume833
Issue number2
DOIs
Publication statusPublished - 20 Dec 2016

Abstract

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}* ˜ {10}9.5-11.5 {M}⊙ , and over a range of impact parameters extending to just beyond the halo virial radius (R vir). 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 R vir, 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 Lyα and 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 Lyα lines. The ratio of the velocity offset to the velocity dispersion for the Lyα absorbers 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 Lyα velocity 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.

    Research areas

  • galaxies: halos, galaxies: star formation, quasars: absorption lines

Download statistics

No data available

ID: 57683995