The B3-VLA CSS sample - VI. VLA images at 2 cm

被引:21
|
作者
Rossetti, A
Fanti, C
Fanti, R
Dallacasa, D
Stanghellini, C
机构
[1] INAF, Ist Radioastron, I-40129 Bologna, Italy
[2] Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy
[3] Univ Bologna, Dipartimento Fis, I-40126 Bologna, Italy
关键词
galaxies : active; galaxies : nuclei; radio continuum : galaxies; galaxies : quasars : general;
D O I
10.1051/0004-6361:20053945
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. New radio observations are presented for a sample of 56 Compact Steep Spectrum (CSS) radio sources from the B3-VLA CSS sample. Methods. We used the VLA A-configuration observation at 2 cm to obtain high-frequency, high-resolution data. Results. The majority (85%) of sources have a double morphology with a number of them showing a large asymmetry in terms of their component flux densities and/or component arm ratio. These new data have revealed 27 cores and core candidates. Three of the sources have a core-jet morphology and the morphologies of a few objects (<= 10%) are still ambiguous. The integrated radio spectra, over a frequency range from 0.16 to 15 GHz, show good agreement with a "continuous injection model" for >= 85% of the sources.
引用
收藏
页码:49 / U37
页数:30
相关论文
共 50 条
  • [1] The B3-VLA CSS sample: VI. VLA images at 2 cm
    Rossetti, A.
    Fanti, C.
    Fanti, R.
    Dallacasa, D.
    Stanghellini, C.
    [J]. Astronomy and Astrophysics, 1600, 449 (01): : 49 - 60
  • [2] The B3-VLA CSS sample II. VLBA images at 18 cm
    [J]. Dallacasa, D. (ddallaca@ira.cnr.it), 1600, EDP Sciences (389):
  • [3] The B3-VLA CSS sample - II. VLBA images at 18 cm
    Dallacasa, D
    Tinti, S
    Fanti, C
    Fanti, R
    Gregorini, L
    Stanghellini, C
    Vigotti, M
    [J]. ASTRONOMY & ASTROPHYSICS, 2002, 389 (01) : 115 - 125
  • [4] The B3-VLA CSS sample - III. EVN & MERLIN images at 18 cm
    Dallacasa, D.
    Fanti, C.
    Giacintucci, S.
    Stanghellini, C.
    Fanti, R.
    Gregorini, L.
    Vigotti, M.
    [J]. 1600, EDP Sciences (389):
  • [5] The B3-VLA CSS sample - III. EVN & MERLIN images at 18 cm
    Dallacasa, D
    Fanti, C
    Giacintucci, S
    Stanghellini, C
    Fanti, R
    Gregorini, L
    Vigotti, M
    [J]. ASTRONOMY & ASTROPHYSICS, 2002, 389 (01) : 126 - 142
  • [6] The B3-VLA CSS sample - V. VLBA images at 6 and 3.6 cm
    Orienti, M
    Dallacasa, D
    Fanti, C
    Fanti, R
    Tinti, S
    Stanghellini, C
    [J]. ASTRONOMY & ASTROPHYSICS, 2004, 426 (02) : 463 - +
  • [7] The B3-VLA CSS sample: Polarisation observations
    Rossetti, A.
    Dallacasa, D.
    Fanti, C.
    Fanti, R.
    Mack, K. -H.
    [J]. ASTRONOMISCHE NACHRICHTEN, 2009, 330 (2-3) : 165 - 166
  • [8] The B3-VLA CSS sample. V. VLBA images at 6 and 3.6 cm
    [J]. Orienti, M. (orienti@ira.cnr.it), 1600, EDP Sciences (426):
  • [9] The B3-VLA Sample
    Vigotti, M.
    Djorgovski, S. G.
    Gregorini, L. et al.
    [J]. International Astronomical Union - Symposium, (175):
  • [10] The B3-VLA sample
    Vigotti, M
    Djorgovski, SG
    Gregorini, L
    Klein, U
    Mack, KH
    Maxfield, L
    Reuter, HP
    Thompson, D
    [J]. EXTRAGALACTIC RADIO SOURCES, 1996, (175): : 519 - 521