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AGN-enhanced outflows of low-ionization gas in star-forming galaxies at 1.7
- Publication Year :
- 2016
- Publisher :
- arXiv, 2016.
-
Abstract
- Fast and energetic winds are invoked by galaxy formation models as essential processes in the evolution of galaxies. These outflows can be powered either by star-formation and/or AGN activity, but the relative dominance of the two mechanisms is still under debate. We use spectroscopic stacking analysis to study the properties of the low-ionization phase of the outflow in a sample of 1330 star-forming galaxies (SFGs) and 79 X-ray detected (42<br />MNRAS in press, 10 figures, 3 tables. Major update with respect to previous version: X-ray Chandra catalogues were upgraded to the latest available versions (Chandra 7Ms and COSMOS-Legacy). The mass-matched sample of SFGs was also re-defined. Major results are unchanged
- Subjects :
- Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Astrophysics::High Energy Astrophysical Phenomena
Astrophysics of Galaxies (astro-ph.GA)
Astrophysics::Solar and Stellar Astrophysics
FOS: Physical sciences
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics::Galaxy Astrophysics
Subjects
Details
- Database :
- OpenAIRE
- Accession number :
- edsair.doi...........0a651cdc74bdb6e9762c91a042a77ae3
- Full Text :
- https://doi.org/10.48550/arxiv.1611.05884