Evidence for a precessing accretion disk in the nucleus of NGC 1097

Thaisa Storchi-Bergmann, Michael Eracleous, Maria Teresa Ruiz, Mario Livio, Andrew S. Wilson, Alexei V. Filippenko

Research output: Contribution to journalArticle

69 Citations (Scopus)

Abstract

We present new spectroscopic observations of the LINER (and now Seyfert 1) nucleus of NGC 1097, and discuss the evolution of its broad, double-peaked Balmer lines. When originally discovered in 1991, the red peak of the double-peaked Hα line was stronger than the blue, while by 1994 the Hα profile had become almost symmetric and the integrated line flux had decreased to half its original value. Our new spectrum, taken in 1996, shows that the broad, double-peaked lines have returned to almost their original strengths, the profiles of Hβ and Hα are identical to within errors, and the broad-line emitting region is unreddened. However, the profile of the Balmer lines is now such that the blue peak is stronger than the red, opposite to the asymmetry observed in 1991. Various models are considered for the observed behavior, all assuming that the emission lines originate in an accretion disk. We present a refined version of the precessing, planar, elliptical accretion-ring model proposed by Storchi-Bergmann et al. and Eracleous et al. This model provides an acceptable fit to the line profiles. We also consider the possibility that the line-profile evolution results from a precessing warp in the disk, induced by irradiation from the center, and show that the range of radii and precession timescales expected in this model are consistent with the observations. The sudden appearance of the "disklike" broad-line profiles in NGC 1097 could have resulted from the formation of a new accretion disk due, for example, to the tidal disruption of a star or the illumination of a preexisting disk by a transient ionizing source at the center of the disk.

Original languageEnglish (US)
Pages (from-to)87-93
Number of pages7
JournalAstrophysical Journal
Volume489
Issue number1 PART I
DOIs
StatePublished - Jan 1 1997

Fingerprint

accretion disks
accretion
nuclei
profiles
precession
H lines
asymmetry
irradiation
timescale
illumination
stars
radii
rings

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Storchi-Bergmann, T., Eracleous, M., Ruiz, M. T., Livio, M., Wilson, A. S., & Filippenko, A. V. (1997). Evidence for a precessing accretion disk in the nucleus of NGC 1097. Astrophysical Journal, 489(1 PART I), 87-93. https://doi.org/10.1086/304783
Storchi-Bergmann, Thaisa ; Eracleous, Michael ; Ruiz, Maria Teresa ; Livio, Mario ; Wilson, Andrew S. ; Filippenko, Alexei V. / Evidence for a precessing accretion disk in the nucleus of NGC 1097. In: Astrophysical Journal. 1997 ; Vol. 489, No. 1 PART I. pp. 87-93.
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Storchi-Bergmann, T, Eracleous, M, Ruiz, MT, Livio, M, Wilson, AS & Filippenko, AV 1997, 'Evidence for a precessing accretion disk in the nucleus of NGC 1097', Astrophysical Journal, vol. 489, no. 1 PART I, pp. 87-93. https://doi.org/10.1086/304783

Evidence for a precessing accretion disk in the nucleus of NGC 1097. / Storchi-Bergmann, Thaisa; Eracleous, Michael; Ruiz, Maria Teresa; Livio, Mario; Wilson, Andrew S.; Filippenko, Alexei V.

In: Astrophysical Journal, Vol. 489, No. 1 PART I, 01.01.1997, p. 87-93.

Research output: Contribution to journalArticle

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Storchi-Bergmann T, Eracleous M, Ruiz MT, Livio M, Wilson AS, Filippenko AV. Evidence for a precessing accretion disk in the nucleus of NGC 1097. Astrophysical Journal. 1997 Jan 1;489(1 PART I):87-93. https://doi.org/10.1086/304783