A candidate tidal disruption event in the Galaxy cluster Abell 3571

作者：Cappelluti N^*; Ajello M; Rebusco P; Komossa S; Bongiorno A; Clemens C; Salvato M; Esquej P; Aldcroft T; Greiner J; Quintana H

来源：Astronomy & Astrophysics, 2009, 495(2): L9-L12.

DOI：10.1051/0004-6361/200811479

• X-rays: galaxies
• galaxies: clusters: individual: Abell 3571
• galaxies: nuclei
• X-rays: bursts
• galaxies: active

Context. Tidal disruption events are possible sources of temporary nuclear activity in galactic nuclei and can be considered as good indicators of the existence of supermassive black holes in the centers of galaxies. Aims. A new X-ray source has been detected serendipitously with ROSAT in a PSPC pointed observation of the galaxy cluster A3571. Given the strong flux decay of the object in subsequent detections, the tidal disruption scenario is investigated as a possible explanation of the event.
Methods. We followed the evolution of the X-ray transient with ROSAT, XMM-Newton and Chandra for a total period of similar to 13 years. We also obtained 7-band optical/NIR photometry with GROND at the ESO/MPI 2.2 m telescope.
Results. We report a very large decay of the X-ray flux of the ROSAT source identified with the galaxy LEDA 095953, a member of the cluster Abell 3571. We measured a maximum 0.3-2.4 keV luminosity Log (L(X)) = 42.8 erg s(-1). The high state of the source lasted at least 150 ks; afterwards L(X) declined as similar to t(-2). The spectrum of the brightest epoch is consistent with a black body with temperature kT similar to 0.12 keV.
Conclusions. The total energy released by this event in 10 yr was estimated to be Delta E > 2 x 10(50) erg. We interpret this event as a tidal disruption of a solar type star by the central supermassive black hole (i.e. similar to 10(7) M(circle dot)) of the galaxy.

• 出版日期2009-2