The B3-VLA CSS sample - II. VLBA images at 18 cm

被引:42
作者
Dallacasa, D
Tinti, S
Fanti, C
Fanti, R
Gregorini, L
Stanghellini, C
Vigotti, M
机构
[1] Univ Bologna, Dipartmento Astron, I-40127 Bologna, Italy
[2] CNR, Ist Radioastron, I-40129 Bologna, Italy
[3] Univ Bologna, Dipartimento Fis, I-40126 Bologna, Italy
[4] CNR, Ist Radioastron, I-96017 Noto, SR, Italy
关键词
galaxies : active; radio continuum : galaxies; quasars : general;
D O I
10.1051/0004-6361:20020576
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
VLBA observations at 18 cm are presented for 28 Compact Steep{spectrum radio Sources (CSSs) from the B3-VLA CSS sample. These sources were unresolved in previous VLA observations at high frequencies or their brightness distribution was dominated by an unresolved steep spectrum component. More than half of them also showed a low frequency turnover in their radio spectrum. The VLBA images display in most cases a compact symmetric structure. Only in a minority of cases complex morphologies are present.
引用
收藏
页码:115 / 125
页数:11
相关论文
共 17 条
[1]  
Baldwin J., 1982, IAU S, V97, P21
[2]  
Begelman M.C., 1996, Cygnus A - Studay of a Radio Galaxy, P209
[3]   The NRAO VLA Sky Survey [J].
Condon, JJ ;
Cotton, WD ;
Greisen, EW ;
Yin, QF ;
Perley, RA ;
Taylor, GB ;
Broderick, JJ .
ASTRONOMICAL JOURNAL, 1998, 115 (05) :1693-1716
[4]   The B3-VLA CSS sample - III. EVN & MERLIN images at 18 cm [J].
Dallacasa, D ;
Fanti, C ;
Giacintucci, S ;
Stanghellini, C ;
Fanti, R ;
Gregorini, L ;
Vigotti, M .
ASTRONOMY & ASTROPHYSICS, 2002, 389 (01) :126-142
[5]  
FANTI C, 1995, ASTRON ASTROPHYS, V302, P317
[6]   Multi-frequency VLA observations of a new sample of CSS/GPS radio sources [J].
Fanti, C ;
Pozzi, F ;
Dallacasa, D ;
Fanti, R ;
Gregorini, L ;
Stanghellini, C ;
Vigotti, M .
ASTRONOMY & ASTROPHYSICS, 2001, 369 (02) :380-420
[7]  
FANTI C, 2000, P 5 EVN S ONS SPAC O
[8]  
FANTI C, 2001, P ISS UN AGNS OSS AS
[9]  
FANTI R, 1990, ASTRON ASTROPHYS, V231, P333
[10]   A self-similar model for extragalactic radio sources [J].
Kaiser, CR ;
Alexander, P .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997, 286 (01) :215-222