A QSO 2.4 arcsec from a dwarf galaxy - the rest of the story
| dc.creator | Arp, Halton | |
| dc.date | 1998-11-12 | |
| dc.date.accessioned | 2026-07-07T02:29:04Z | |
| dc.date.available | 2026-07-07T02:29:04Z | |
| dc.description | D. Reimers and H.-J. Hagen report in A&A 329, L25 (1998) that a QSO of z = .807 is a "by chance projection" on the center of a galaxy of z = .009. A considerable amount of previously published evidence would lead us to expect an active, low redshift galaxy within about one degree of such a quasar. It is shown here that, in fact, there is a bright Seyfert galaxy of z = .008 only 36.9 arcmin distance. Moreover, it turns out that a total of five quasars, plus the dwarf galaxy, are accurately aligned along the minor axis of this Seyfert with the quasars in descending order of redshift, i.e., z = 2.13, 1.97, .81, .69 and .35. | |
| dc.description | 4 pages, 3 figures, to appear in A&A Letters | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9811191 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9811191 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/13326 | |
| dc.subject | Astrophysics | |
| dc.title | A QSO 2.4 arcsec from a dwarf galaxy - the rest of the story | |
| dc.type | text |