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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 731861.0, MPI für Astronomie / Publikationen_mpia
Revealing the nature of extreme coronal-line emitter SDSS J095209.56+214313.3
Authors:Palaversa, L.; Gezari, S.; Sesar, B.; Stuart, J. S.; Wozniak, P.; Holl, B.; Ivezić, Ž.
Date of Publication (YYYY-MM-DD):2016
Title of Journal:The Astrophysical Journal
Volume:819
Issue / Number:2
Start Page:id. 151 (7 pp)
Audience:Not Specified
Abstract / Description:Extreme coronal-line emitter (ECLE) SDSS J095209.56+214313.3, known by its strong, fading, high-ionization lines, has been a long-standing candidate for a tidal disruption event however, a supernova (SN) origin has not yet been ruled out. Here we add several new pieces of information to the puzzle of the nature of the transient that powered its variable coronal lines: (1) an optical light curve from the Lincoln Near Earth Asteroid Research (LINEAR) survey that serendipitously catches the optical flare, and (2) late-time observations of the host galaxy with the Swift Ultraviolet and Optical Telescope (UVOT) and X-ray telescope (XRT) and the ground-based Mercator telescope. The well-sampled, ∼10 yr long, unfiltered LINEAR light curve constrains the onset of the flare to a precision of ±5 days and enables us to place a lower limit on the peak optical magnitude. Difference imaging allows us to estimate the location of the flare in proximity of the host galaxy core. Comparison of the GALEX data (early 2006) with the recently acquired Swift UVOT (2015 June) and Mercator observations (2015 April) demonstrates a decrease in the UV flux over a ∼10 yr period, confirming that the flare was UV-bright. The long-lived UV-bright emission, detected 1.8 rest-frame years after the start of the flare, strongly disfavors an SN origin. These new data allow us to conclude that the flare was indeed powered by the tidal disruption of a star by a supermassive black hole and that tidal disruption events are in fact capable of powering the enigmatic class of ECLEs.
Free Keywords:black hole physics; circumstellar matter; galaxies: individual: SDSS J095209.56+214313.3; galaxies: nuclei; supernovae: general; ultraviolet: galaxies
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:ISSN:0004-637X %R 10.3847/0004-637X/819/2/151
URL:http://adsabs.harvard.edu/abs/2016ApJ...819..151P
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