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A&A 391, 833-840 (2002)
DOI: 10.1051/0004-6361:20020828
NGC 3628: Ejection activity associated with quasars
H. Arp1, E. M. Burbidge2, Y. Chu3, E. Flesch4, F. Patat5 and G. Rupprecht51 Max-Planck-Institut für Astrophysik, 85741 Garching, Germany
2 Center for Astrophysics and Space Sciences, University of California, San Diego, La Jolla, CA 92093-0424, USA
3 Center for Astrophysics, University of Science and Technology, Hefei, Anhui, 230026, PR China
4 PO Box 12520, Wellington, New Zealand
5 European Southern Observatory, 85748 Garching, Germany
(Received 20 March 2002 / Accepted 3 June 2002 )
Abstract
NGC 3628 is a well-studied starburst/low level AGN galaxy in the Leo
Triplet noted for its extensive outgassed plumes of neutral hydrogen. QSOs
are shown to be concentrated around NGC 3628 and aligned with the HI
plumes. The closest high redshift quasar has
z=2.15 and is at the
tip of an X-ray filament emerging along the minor axis HI plume.
Location
at this point has an accidental probability of ~
. In
addition a coincident chain of optical objects coming out along the
minor axis ends on this quasar.
Key words: galaxies: active -- galaxies: individual: NGC 3628 -- quasars: general -- radio lines: galaxies -- X-rays: galaxies
Offprint request: H. Arp, arp@mpa-garching.mpg.de
SIMBAD Objects
© ESO 2002
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