Hostname: page-component-76fb5796d-45l2p Total loading time: 0 Render date: 2024-04-25T16:39:42.367Z Has data issue: false hasContentIssue false

Space VLBI

Published online by Cambridge University Press:  13 May 2016

H. Hirabayashi*
Affiliation:
Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan

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.

Space VLBI enables high angular resolution and high dynamic range imaging through an extension of ground-based VLBI. The TDRSS space VLBI experiments in the 1980s were followed by the first space VLBI imaging mission, VSOP, in the 1990s. The new century holds the promise of the VSOP-2 and ARISE missions, which aim for more sensitive, higher angular resolution and higher observing frequency capabilities. These missions will enable AGNs to be viewed much more clearly and will make broader science areas, including lower brightness sources, accessible. It is noted that in all space VLBI missions, international collaboration in global sense plays an important role.

Type
Prospects for High Angular Resolution Instrumentation
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Bolton, J.G. & Stanley, G.J. 1948, Nature, 161, 312.Google Scholar
Burke, B.F. 1984, in VLBI and Compact Radio Sources, ed Fanti, R., Kellermann, K., Setti, G., IAU Symp. 110, 397.Google Scholar
Hirabayashi, H. et al. 1998, Science. 281, 1825.Google Scholar
Hirabayashi, H., Hirosawa, H. et al. 2000a, PASJ in press.Google Scholar
Hirabayashi, H., Fomalont, E.B. et al. 2000b, PASJ in press.Google Scholar
Hirabayashi, H. et al. 2000c, in Astrophysical Phenomena Revealed by Space VLBI, ed. Hirabayashi, H., Edwards, P. G. & Murphy, D. W., (Sagamihara: ISAS) 277.Google Scholar
Hirabayashi, H. et al. 2001, these proceedings.Google Scholar
Jones, D.L. et al. 2000, in Astrophysical Phenomena Revealed by Space VLBI, ed. Hirabayashi, H., Edwards, P. G. & Murphy, D. W., (Sagamihara: ISAS) 265.Google Scholar
Kardashev, N.S. 1997, Exp. Astron. 7, 329.CrossRefGoogle Scholar
Kardashev, N.S., Slysh, V.I. 1988, in The Impact of VLBI on Astrophysics and Geophysics, ed Reid, M.J., Moran, J.M., IAU Symp. 129, 433.Google Scholar
Kobayashi, H., Shimoikura, T. et al. 2000, in Astrophysical Phenomena Revealed by Space VLBI, ed. Hirabayashi, H., Edwards, P. G. & Murphy, D. W., (Sagamihara: ISAS) 109.Google Scholar
Levy, G.S., Linfield, R.P., Ulvestad, J.S., Edwards, C.D., Jordan, F.J., DiNardo, S.J., Christensen, C.S., Preston, R.A. et al. 1986, Science 234, 187.Google Scholar
Linfield, R.P., Levy, G.S., Ulvestad, J.S., Edwards, C.D., DiNardo, S.J., Stavert, L.R., Ottenhoff, C.H., Whitney, A.R. et al. 1989, ApJ 336, 1105.Google Scholar
Linfield, R.P., Levy, G.S., Edwards, C.D., Ulvestad, J.S., Ottenhoff, C.H., Hirabayashi, H., Morimoto, M., Inoue, M. et al. 1990, ApJ 358, 350.CrossRefGoogle Scholar
Marscher, A.P. 2000, in Astrophysical Phenomena Revealed by Space VLBI, ed. Hirabayashi, H., Edwards, P. G. & Murphy, D. W., (Sagamihara: ISAS) 261.Google Scholar
Meier, D.L. & Koide, S. 2000, in Astrophysical Phenomena Revealed by Space VLBI, ed. Hirabayashi, H., Edwards, P. G. & Murphy, D. W., (Sagamihara: ISAS) 31.Google Scholar
Murata, Y., Hirabayashi, H. & Edwards, P.G. 2001, these proceedings.Google Scholar
Pilbratt, G. 1991, in Radio Interferometry: Theory, Techniques, and Applications, ed Cornwell, T.J., Perley, R.A., ASP Conf. Ser. 19, 102.Google Scholar
Schilizzi, R.T. 1988, in The Impact of VLBI on Astrophysics and Geophysics, ed Reid, M.J., Moran, J.M., IAU Symp. 129, 441.Google Scholar
Shibata, K. 2000, in Astrophysical Phenomena Revealed by Space VLBI, ed. Hirabayashi, H., Edwards, P. G. & Murphy, D. W., (Sagamihara: ISAS) 29.Google Scholar
Tanaka, Y., Nandra, K., Fabian, A.C. et al. 1995, Nature, 375, 659.Google Scholar
Ulvestad, J.S. 2000, Adv. Space Res. 26, 735.Google Scholar
Ulvestad, J.S. & Linfield, R.P. 1998, IAU Colloquium 164, ASP Conf. Series, 144, 397.Google Scholar