THE COS-HALOS SURVEY: AN EMPIRICAL DESCRIPTION OF METAL-LINE ABSORPTION IN THE LOW-REDSHIFT CIRCUMGALACTIC MEDIUM

Journal Article · Fri Feb 15 04:00:00 EST 2013 · Astrophysical Journal, Supplement Series

DOI:https://doi.org/10.1088/0067-0049/204/2/17· OSTI ID:22107746

Werk, Jessica K.; Prochaska, J. Xavier ^[1]; Thom, Christopher; Tumlinson, Jason ^[2]; Tripp, Todd M. ^[3]; O'Meara, John M. ^[4]

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1. UCO/Lick Observatory, University of California, Santa Cruz, CA (United States)
2. Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD (United States)
3. Department of Astronomy, University of Massachusetts, Amherst, MA (United States)
4. Department of Chemistry and Physics, Saint Michael's College, Colchester, VT (United States)

We present the equivalent width and column density measurements for low and intermediate ionization states of the circumgalactic medium (CGM) surrounding 44 low-z, L Almost-Equal-To L* galaxies drawn from the COS-Halos survey. These measurements are derived from far-UV transitions observed in HST/COS and Keck/HIRES spectra of background quasars within an impact parameter R < 160 kpc to the targeted galaxies. The data show significant metal-line absorption for 33 of the 44 galaxies, including quiescent systems, revealing the common occurrence of a cool (T Almost-Equal-To 10{sup 4}-10{sup 5} K), metal-enriched CGM. The detection rates and column densities derived for these metal lines decrease with increasing impact parameter, a trend we interpret as a declining metal surface density profile for the CGM. A comparison of the relative column densities of adjacent ionization states indicates that the gas is predominantly ionized. The large surface density in metals demands a large reservoir of metals and gas in the cool CGM (very conservatively, M {sup cool} {sub CGM} > 10{sup 9} M {sub Sun }), which likely traces a distinct density and/or temperature regime from the highly ionized CGM traced by O{sup +5} absorption. The large dispersion in absorption strengths (including non-detections) suggests that the cool CGM traces a wide range of densities or a mix of local ionizing conditions. Lastly, the kinematics inferred from the metal-line profiles are consistent with the cool CGM being bound to the dark matter halos hosting the galaxies; this gas may serve as fuel for future star formation. Future work will leverage this data set to provide estimates on the mass, metallicity, dynamics, and origin of the cool CGM in low-z, L* galaxies.

• OSTI ID: 22107746
• Journal Information: Astrophysical Journal, Supplement Series, Journal Name: Astrophysical Journal, Supplement Series Journal Issue: 2 Vol. 204; ISSN 0067-0049; ISSN APJSA2
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
ABSORPTION
DETECTION
DISPERSIONS
GALAXIES
IMPACT PARAMETER
IONIZATION
MASS
MATTER
RED SHIFT
STARS