z-logo
open-access-imgOpen Access
MCG +00‐32‐16: An Irregular Galaxy Close to the Lowest Redshift Absorber on the 3C 273 Line of Sight
Author(s) -
G. L. Hoffman,
N. Lu,
E. E. Salpeter,
Bryan M. Connell,
Rene FromholdTreu
Publication year - 1998
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/305765
Subject(s) - physics , redshift , astrophysics , galaxy , quasar , milky way , line of sight , photometry (optics) , astronomy , stars
MCG+00-32-16 is the galaxy closest in position-velocity space to the lowestredshift Ly$\alpha$ absorber along the line-of-sight to the quasar 3C 273. Itsprojected separation is 204 (d/19 Mpc) kpc, where d is the distance from theMilky Way to the galaxy, and the redshift difference is only 94 km/s; HI1225+01 is slightly closer in projected separation to the absorber, but has agreater redshift difference. We present HI synthesis array mapping and CCDphotometry in B and R for MCG+00-32-16. The HI disk is rotating in such a waythat the side of the galaxy closer to the sight-line to the quasar has thelarger velocity difference from the absorber. The absorber may be a ``faileddwarf'' member of a poor galaxy group of which MCG+00-32-16 and HI 1225+01 arethe only members to have formed stars.Comment: 14 pages, 9 figures, accepted by Astrophysical Journa

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom