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HST Observations Reveal the Curious Geometry of Circumgalactic Gas.

Authors :
Kacprzak, Glenn G.
Muzahid, Sowgat
Churchill, Christopher W.
Nielsen, Nikole M.
Charlton, Jane C.
Gil de Paz, Armando
Knapen, Johan H.
Lee, Janice C.
Source :
Proceedings of the International Astronomical Union; 2016 Supplement S321, Vol. 11, p342-344, 3p
Publication Year :
2016

Abstract

We have discovered that warm gas flows along galaxy major and minor axes detected out to 200 kpc. Our results are derived from a sample of HST-imaged isolated galaxies with nearby background quasars used to probe their 105K CGM detected in HST/COS UV spectra (traced by Ovi absorption). We constrain the geometry of the gas to reside between 20-40 degrees of the projected major axis and within 60 degrees of the projected minor axis, with little-to-no gas found in between. Furthermore, strong absorption systems tend to be found along the minor axes of star-forming galaxies. All of our results are consistent with the current view of the CGM originating from major axis-fed inflows/recycled gas and from minor axis-driven outflows. [ABSTRACT FROM PUBLISHER]

Details

Language :
English
ISSN :
17439213
Volume :
11
Database :
Complementary Index
Journal :
Proceedings of the International Astronomical Union
Publication Type :
Academic Journal
Accession number :
121995274
Full Text :
https://doi.org/10.1017/S1743921316008905