Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-29T11:45:12.102Z Has data issue: false hasContentIssue false

Millimeter-Wave VLBI Observations of Compact Steep-Spectrum Radio Sources

Published online by Cambridge University Press:  12 April 2016

S. Kameno
Affiliation:
Astronomy Department, The University of Tokyo, Bunkyo-ku, Tokyo 113
M. Inoue
Affiliation:
Nobeyama Radio Observatory, Minamimaki-mura, Minamisaku-gun, Nagano 384-13
H. Takaba
Affiliation:
Kashima Space Research Center, 893-1 Hirai, Kashima, Ibaraki 314
T. Iwata
Affiliation:
Kashima Space Research Center, 893-1 Hirai, Kashima, Ibaraki 314
Y. Takahashi
Affiliation:
Kashima Space Research Center, 893-1 Hirai, Kashima, Ibaraki 314
R. Nan
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijin
R. T. Schilizzi
Affiliation:
Radiosterrewatcht Dwingeloo, Postbus 2, 7990 AA Dwingeloo

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We report the observations of compact steep-spectrum radio sources (CSSs) by VLBI at 22 and 43 GHz and single dich at 22, 43, and 92 GHz. Our results show that CSS also has an active core as well as other AGNs.

Type
1. Recent Developments and Upgrading Plans for the Near Future
Copyright
Copyright © Astronomical Society of the Pacific 1994

References

Fanti, C. et al. 1985, A&A, 143, 292.Google Scholar
Fanti, R. et al. 1990, A&A, 231, 333.Google Scholar
Kameno, S. et al. 1992, in Sub-Arcsecond Radio Astronomy, Conference Held at the Univ. of Manchester.Google Scholar
Preston, R. A. et al. 1985, AJ, 90, 1599.CrossRefGoogle Scholar
Saikia, D. J. 1989, in Miller, H. R., Witta, P. J. (eds.) Active Galactic Nuclei, Springer-Verlag, P. 317 Google Scholar
Steppe, H. et al. 1990, in Fanti, C. et al. (eds.) Compact Steep-Spectrum and GHz-Peaked Spectrum Radio Sources. Consiglio Nazionale delle Ricerche Istituto di Radioastronomia, Bologna Google Scholar