SDSS J092712.65+294344.0: RECOILING BLACK HOLE OR A SUBPARSEC BINARY CANDIDATE?

Journal Article · Wed May 20 04:00:00 EDT 2009 · Astrophysical Journal

DOI:https://doi.org/10.1088/0004-637X/697/1/288; COUNTRY OF INPUT: INTERNATIONAL ATOMIC ENERGY AGENCY (IAEA)· OSTI ID:21300576

Bogdanovic, Tamara ^[1]; Eracleous, Michael; Sigurdsson, Steinn ^[2]

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1. Department of Astronomy, University of Maryland, College Park, MD 20742-2421 (United States)
2. Department of Astronomy and Astrophysics and Center for Gravitational Wave Physics, Pennsylvania State University, University Park, PA 16802 (United States)

A search for recoiling supermassive black hole (SBH) candidates recently yielded the best candidate thus far, SDSS J092712.65+294344.0 reported by Komossa et al. Here we propose the alternative hypothesis that this object is an SBH binary. From the velocity shift imprinted in the emission-line spectrum we infer an orbital period of {approx}190 years for a binary mass ratio of 0.1, a secondary black hole mass of 10{sup 8} M {sub sun}, and assuming inclination and orbital phase angles of 45 deg. In this model the origin of the blueshifted narrow emission lines is naturally explained in the context of an accretion flow within the inner rim of the circumbinary disk. We attribute the blueshifted broad emission lines to gas associated with a disk around the accreting secondary black hole. We show that, within the uncertainties, this binary system can be long lived and thus, is not observed in a special moment in time. The orbital motion of the binary can potentially be observed with the VLBA if at least the secondary black hole is a radio emitter. In addition, for the parameters quoted above, the orbital motion will result in a {approx}100 km s{sup -1} velocity shift of the emission lines on a timescale of about a year, providing a direct observational test for the binary hypothesis.

• OSTI ID: 21300576
• Journal Information: Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 697; ISSN ASJOAB; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
99 GENERAL AND MISCELLANEOUS
BLACK HOLES
EMISSION
GALAXIES
GALAXY NUCLEI
INCLINATION
QUASARS
VELOCITY