REVEALING THE NATURE OF EXTREME CORONAL-LINE EMITTER SDSS J095209.56+214313.3

REVEALING THE NATURE OF EXTREME CORONAL-LINE EMITTER SDSS J095209.56+214313.3

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...

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Bibliographic Details
Main Authors: Palaversa, Lovro (Author), Gezari, Suvi (Author), Sesar, Branimir (Author), Wozniak, Przemyslaw (Author), Holl, Berry (Author), Ivezić, Željko (Author), Stuart, J. Scott (Contributor)
Other Authors: Lincoln Laboratory (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2017-04-20T19:08:20Z.
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