A Seyfert Nucleus in BL Lacertae

Axon, D.J., Corbett, E.A., Robinson, A. and Hough, J. (1999) A Seyfert Nucleus in BL Lacertae. In: UNSPECIFIED.

Copy

We have obtained spectroscopic observations of the broad Ha line in BL Lacertae over a period of 30 months. These data show that the line equivalent width is anti-correlated with the continuum flux implying that the broad line emission is not powered primarily by synchrotron emission from the relativistic jet. The most probable explanation is that the broad line region in BL Lacertae is photoionized by continuum emission from an accretion disk which at optical wavelengths is dominated by the Doppler beamed synchroton continuum.

Item Type	Conference or Workshop Item (Other)
Additional information	Original paper can be found at: http://161.58.115.79/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific
Date Deposited	15 May 2025 16:19
Last Modified	10 Jul 2025 23:22