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FeLoBAL quasars: evolution, orientation or just oddBALs?

Published online by Cambridge University Press:  12 September 2016

Daniel Lawther
Affiliation:
Dark Cosmology Centre, Niels Bohr Institutet, Denmark email: danielpe@dark-cosmology.dk
Marianne Vestergaard
Affiliation:
Dark Cosmology Centre, Niels Bohr Institutet, Denmark email: danielpe@dark-cosmology.dk Steward Observatory, University of Arizona, USA
Xiaohui Fan
Affiliation:
Steward Observatory, University of Arizona, USA
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Abstract

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FeLoBAL quasars may be an early evolutionary stage of merger-triggered quasar activity. We test this hypothesis using HST imaging of four FeLoBAL quasars. The host galaxy colors are consistent with early-type quiescent galaxies or heavily-obscured starbursts.

Type
Poster Papers
Copyright
Copyright © International Astronomical Union 2016 

References

Barden, M., Jahnke, K. and Häussler, B. 2008, ApJS, 175, 105B CrossRefGoogle Scholar
Elvis, M. 2012, ASPC, v.460, p.186E Google Scholar
Hall, P.B. et al., 2002, ApJS, 141, 267H Google Scholar
Peng, et al. 2010, AJ, 139, 2097 Google Scholar
Urry, C.M. and Padovani, P. 1995, PASP, v.107, p.803 Google Scholar
Voit, G. M., Weymann, R. J. and Korista, K. T. 1993, ApJ, 413, 95V Google Scholar