SIMBAD references

2022MNRAS.517L..71Z - Mon. Not. R. Astron. Soc., 517, L71-L75 (2022/November-3)

Modelling the flare in NGC 1097 from 1991 to 2004 as a tidal disruption event.

ZHANG X.-G.

Abstract (from CDS):

In the letter, interesting evidence is reported to support a central tidal disruption event (TDE) in the known AGN NGC 1097. Considering the motivations of TDE as one probable origination of emission materials of double-peaked broad emission lines and also as one probable explanation to changing-look AGN, it is interesting to check whether there are clues to support a TDE in NGC 1097, not only a changing-look AGN but also an AGN with double-peaked broad emission lines. Under the assumption that the onset of broad Hα emission was due to a TDE, the 13 yr-long (1991-2004) variability of double-peaked broad Hα line flux in NGC 1097 can be well predicted by theoretical TDE model, with a (1 - 1.5) M⊙ main-sequence star tidally disrupted by the central BH with TDE model determined mass about (5 - 8) × 107 M⊙. The results provide interesting evidence to not only support TDE-related origin of double-peaked broad line emission materials but also support TDE as an accepted physical explanation to physical properties of changing-look AGN.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): galaxies: active - galaxies: nuclei - quasars: emission lines - quasars: individual (NGC 1097) - galaxies: Seyfert

Simbad objects: 10

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