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Published November 1, 2012 | Published
Journal Article Open

SDSS 0956+5128: A Broad-line Quasar with Extreme Velocity Offsets

Abstract

We report on the discovery of a Type 1 quasar, SDSS 0956+5128, with a surprising combination of extreme velocity offsets. SDSS 0956+5128 is a broad-lined quasar exhibiting emission lines at three substantially different redshifts: a systemic redshift of z ~ 0.714 based on narrow emission lines, a broad Mg II emission line centered 1200 km s^(–1) bluer than the systemic velocity, at z ~ 0.707, and broad Hα and Hβ emission lines centered at z ~ 0.690. The Balmer line peaks are 4100 km s^(–1) bluer than the systemic redshift. There are no previously known objects with such an extreme difference between broad Mg II and broad Balmer emission. The two most promising explanations are either an extreme disk emitter or a high-velocity black hole recoil. However, neither explanation appears able to explain all of the observed features of SDSS 0956+5128, so the object may provide a challenge to our general understanding of quasar physics.

Additional Information

© 2012 American Astronomical Society. Received 2012 June 20; accepted 2012 September 4; published 2012 October 12. The authors thank Kevin Bundy, Masahiro Fukugita, Pat Hall, Daniel Proga, Robert Quimby, Allan Sadun, Masayuki Tanaka, and Alexander Tchekhovskoy for valuable comments. This work was supported by the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan. M.A.S., P.P., and R.A. acknowledge the support of NSF grant AST-0707266. C.L.S. and M.E. thank the Aspen Center for Physics and the NSF Grant No. 1066293 for hospitality during the editing of this paper.

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