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
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).