THE MOLONGLO-REFERENCE-CATALOG 1 JY RADIO-SOURCE SURVEY - II - RADIO STRUCTURES OF GALAXY IDENTIFICATIONS

Citation
Vk. Kapahi et al., THE MOLONGLO-REFERENCE-CATALOG 1 JY RADIO-SOURCE SURVEY - II - RADIO STRUCTURES OF GALAXY IDENTIFICATIONS, The Astrophysical journal. Supplement series, 118(2), 1998, pp. 275-326
Citations number
63
Categorie Soggetti
Astronomy & Astrophysics
ISSN journal
00670049
Volume
118
Issue
2
Year of publication
1998
Pages
275 - 326
Database
ISI
SICI code
0067-0049(1998)118:2<275:TM1JRS>2.0.ZU;2-S
Abstract
This is the second in a series of papers discussing the radio, optical , and near-IR properties of a large and complete sample of radio sourc es selected from the Molonglo Reference Catalog (MRC) at 408 MHz. The sample consists of 557 radio sources from the MRC that have S(0.408)gr eater than or equal to 0.95 Jy, -30 degrees < delta < -20 degrees, and \b\ greater than or equal to 20 degrees but excluding the right ascen sion range of 14(h)03(m)-20(h)20(m). While 111 of these are identified with quasars (including six with BL Lac objects), a vast majority of the rest are identified with galaxies. Only a small fraction (less tha n or similar to 2%) appear to have no optical or near-IR counterparts down to an r magnitude of similar to 24 or a K magnitude of similar to 19. A similar fraction have ambiguous identifications. This paper pre sents the radio structures of the 446 radio sources in the sample that are either identified with galaxies or that have remained unidentifie d. Most of the structural information given in the paper is based on h igh-resolution (similar to 1 ''-10 '') observations made with the Very Large Array at a frequency of 4.86 GHz. Several of the large or diffu se sources were also observed at 1.41 GHz. Contour plots of the radio images are also presented for the well-resolved sources. A substantial fraction (similar to 20%) of the sources in the galaxy sample is foun d to be of the ''compact steep spectrum'' variety with alpha(0.408)(4. 86) > 0.5 and linear size l less than or similar to 20 kpc (for H-0 = 50 km s(-1) Mpc(-1); q(0) = 0.5).