A High-Frequency QPO in a Narrow Line Seyfert 1 Galaxy RE J1034+396

Details A High-Frequency QPO in a Narrow Line Seyfert 1 Galaxy RE J1034+396 A High-Frequency QPO in a Narrow Line Seyfert 1 Galaxy RE J1034+396

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..408..303b&link_type=abstract

The Starburst-AGN Connection. ASP Conference Series, Vol. 408, proceedings of the conference held 27-31 October 2008, at Shangha

Astronomy and Astrophysics

Astronomy

1

Scientific paper

With the simple stellar population synthesis to model the stellar contribution in the optical spectrum of a narrow line Seyfert 1 galaxy RE J1034+396, we find that its stellar velocity dispersion is 72kms with an uncertainty less than 8 kms. The black hole mass is 2.2× 10^6 msun if it follows the mbh-σ relation. The mass determination suggests that its X-ray quasi-periodic oscillations(QPOs) given by Gierlinski et al. belongs to a high-frequency QPO.

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