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The variability of the double-peaked Balmer lines in the active nucleus of NGC 1097
1995; IOP Publishing; Volume: 443; Linguagem: Inglês
10.1086/175553
ISSN1538-4357
AutoresThaisa Storchi‐Bergmann, Michael Eracleous, Mario Livio, A. S. Wilson, A. V. Filippenko, J. P. Halpern,
Tópico(s)Galaxies: Formation, Evolution, Phenomena
Resumoview Abstract Citations (87) References (32) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Variability of the Double-peaked Balmer Lines in the Active Nucleus of NGC 1097 Storchi-Bergmann, Thaisa ; Eracleous, Michael ; Livio, Mario ; Wilson, Andrew S. ; Filippenko, Alexei V. ; Halpern, Jules P. Abstract We present spectroscopic observations of the nucleus of the Seyfert/low-ionization nuclear emission-line region galaxy NGC 1097 spanning the period 1991-1994. The goal was to monitor anticipated variations of the broad, double-peaked Balmer lines which appeared abruptly in 1991. We find that the broad Balmer lines have varied significantly over the monitoring period, both in their integrated fluxes and in their profile shapes. The integrated Hα flux has decreased by a factor of 2, the Hα/Hβ ratio has increased, and the originally asymmetric Hα profile has become symmetric. The decline of the Hα flux and the change in the Hα/Hβ ratio can be interpreted as consequences of either increased obscuration along the line of sight, or a decline in the ionizing continuum, but neither of these scenarios can account for the change in profile shapes. A model attributing the line emission to a precessing elliptical ring around a 10^6^ M_sun_ nuclear black hole can reproduce the observed profile variations. In this scenario, the line-emitting ring is the result of the tidal disruption of a star by the black hole. Alternative scenarios associating the broad-line emission with a collimated bipolar outflow also remain viable, but binary black holes and inhomogeneous accretion disks are disfavored by the observed pattern of variability. Publication: The Astrophysical Journal Pub Date: April 1995 DOI: 10.1086/175553 Bibcode: 1995ApJ...443..617S Keywords: Active Galactic Nuclei; Astronomical Models; Balmer Series; H Alpha Line; H Beta Line; Line Shape; Seyfert Galaxies; Variability; Accretion Disks; Astronomical Observatories; Astronomical Spectroscopy; Black Holes (Astronomy); Flux (Rate); Gas Flow; Interstellar Extinction; Ionization; Astrophysics; GALAXIES: INDIVIDUAL NGC NUMBER: NGC 1097; GALAXIES: NUCLEI; GALAXIES: SEYFERT; LINE: PROFILES full text sources ADS | data products SIMBAD (2) NED (1)
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