Volume 379, Number 3, December I 2001
|Page(s)||860 - 863|
|Section||Cosmology (including clusters of galaxies)|
|Published online||15 December 2001|
A pair of Seyferts identified from a ROSAT bright source
National Astronomical Observatories, Chinese Academy of Sciences, A20 Datun Road, Beijing 100012, China
2 Department of Physics, Nanjing Normal University, Nanjing 210097, China
3 Department of Astronomy, Beijing Normal University, Beijing 100875, China
4 Max-Planck-Institute für Extraterrestrische Physik, 85740 Garching, Germany
5 Kitt Peak National Observatory, NOAO, Tucson, AZ85726-6732, USA
Corresponding author: J. -H. Wu, firstname.lastname@example.org
Accepted: 26 September 2001
We report the discovery of a pair of Seyfert galaxies identified in the ROSAT bright source, 1RXS J000306.3-041932. The two Seyferts have the same redshift of 0.106. The angular distance between them is , corresponding to a projected separation of kpc, and suggesting an interacting system. We argue, from its weak IR emission and relatively large nuclear separation, that the system is an example of the interaction between AGNs, rather than interaction-triggered AGN activity.
Key words: galaxies: interactions / galaxies: Seyfert / X-rays: galaxies
© ESO, 2001
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.