LBQS 0103-2753: A 0.3 Arcsec Binary Quasar

Details LBQS 0103-2753: A 0.3 Arcsec Binary Quasar LBQS 0103-2753: A 0.3 Arcsec Binary Quasar

2001-02-28

arxiv.org/abs/astro-ph/0102501v1

The Astrophysical Journal, 549:L155-L159, 2001 March 10

Astronomy and Astrophysics

Astrophysics

12 pages LATEX with 3 EPS figures; uses aaspp4.sty. Accepted for publication in The Astrophysical Journal Letters, volume 550

Scientific paper

10.1086/319173

Imaging and spectroscopy with HST show that LBQS 0103-2753 (V = 17.8, z = 0.848) is a binary quasar with a separation of 0.3 arcsec or 2.3 kpc. This is by far the smallest separation binary quasar reported to date. The two components have very different spectra, including the presence of strong broad absorption lines (BALs) in component A only. The emission-line redshifts, based on the broad high ionization C IV lines, are z_A = 0.834 and z_B = 0.858; their difference is 3900 km/s in velocity units. The broad C IV lines, however, are probably not a good indicator of systemic redshift; and LBQS 0103-2753 A and B could have a much smaller systemic redshift difference, like the other known binary quasars. If the systemic redshift difference is small, then LBQS 0103-2753 would most likely be a galaxy merger that has led to a binary supermassive black hole. There is now one known 0.3 arcsec binary among roughly 500 QSOs that have been observed in a way that would reveal such a close binary. This suggests that QSO activity is substantially more likely for black hole binaries at spacings ~2 kpc than at ~15 to 60 kpc. Between 1987 and 1998, the observed Mg II BAL disappeared.

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