Spectral Monitoring of AGN: Preliminary Results for Ark 564 and Arp 102B

Spectral Monitoring of AGN: Preliminary Results for Ark 564 and Arp 102B

We present preliminary results of the long-term spectral monitoring of two active galactic nuclei with different broad line shapes: Ark 564 and Arp 102B. Ark 564 is a bright nearby narrow-line Syfert 1 (NLS1) galaxy with relatively narrow permitted optical emission lines and a high Fe II/Hβ ratio, w...

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Bibliographic Details
Main Authors: Shapovalova A. I., Popović L. Č., Ilić D., Kovačević A., Kovačević J., Burenkov A. N., Chavushyan V. H.
Format: Article
Language:English
Published: De Gruyter 2011-09-01
Series:Open Astronomy
Subjects:
galaxies active
seyfert
individual ark 564
arp 102b
Online Access:https://doi.org/10.1515/astro-2017-0323
Description
Summary:We present preliminary results of the long-term spectral monitoring of two active galactic nuclei with different broad line shapes: Ark 564 and Arp 102B. Ark 564 is a bright nearby narrow-line Syfert 1 (NLS1) galaxy with relatively narrow permitted optical emission lines and a high Fe II/Hβ ratio, while Arp 102B is a nearby broad-line radio galaxy with broad double-peaked Balmer emission lines. The spectra of Ark 564 were observed during 11-year period (1999-2009) and the spectra of Arp 102B in the 12-year period (1998-2009), with SAO 6 m and 1 m telescopes (Russia) and the OAGH 2.1 m telescope (Cananea, Mexico).
ISSN:2543-6376

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