SIMBAD references

2017ApJ...851L..47G - Astrophys. J., 851, L47-L47 (2017/December-3)

X-ray brightening and UV fading of tidal disruption event ASASSN-15oi.

GEZARI S., CENKO S.B. and ARCAVI I.

Abstract (from CDS):

We present late-time observations by Swift and XMM-Newton of the tidal disruption event (TDE) ASASSN-15oi that reveal that the source brightened in the X-rays by a factor of ∼10 one year after its discovery, while it faded in the UV/optical by a factor of ∼100. The XMM-Newton observations measure a soft X-ray blackbody component with kTbb∼45 eV, corresponding to radiation from several gravitational radii of a central ∼106 M black hole. The last Swift epoch taken almost 600 days after discovery shows that the X-ray source has faded back to its levels during the UV/optical peak. The timescale of the X-ray brightening suggests that the X-ray emission could be coming from delayed accretion through a newly forming debris disk and that the prompt UV/optical emission is from the prior circularization of the disk through stream-stream collisions. The lack of spectral evolution during the X-ray brightening disfavors ionization breakout of a TDE "veiled" by obscuring material. This is the first time a TDE has been shown to have a delayed peak in soft X-rays relative to the UV/optical peak, which may be the first clear signature of the real-time assembly of a nascent accretion disk, and provides strong evidence for the origin of the UV/optical emission from circularization, as opposed to reprocessed emission of accretion radiation.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): accretion, accretion disks - black hole physics - galaxies: nuclei - galaxies: nuclei

Simbad objects: 9

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2017ApJ...851L..47G and select 'bookmark this link' or equivalent in the popup menu


2021.05.07-13:30:13

© Université de Strasbourg/CNRS

    • Contact