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MMVLBI

Published online by Cambridge University Press:  12 April 2016

Lars B. Bååth
Lars B. Bååth*
Affiliation:
Onsala Space Observatory, S-439 92 Onsala, Sweden

Abstract

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VLBI has now made its breakthrough into the mm-wavelength region and is becoming a viable and important new instrument. In this talk I aim to convince you that VLBI will be an important user of your instruments in the future.

Type
1. Recent Developments and Upgrading Plans for the Near Future
Information
International Astronomical Union Colloquium , Volume 140: Astronomy with Millimeter and Submillimeter Wave Interferometry , 1994 , pp. 44 - 49
Copyright
Copyright © Astronomical Society of the Pacific 1994

References

Bååth, L. B., Rogers, A.E.E., Inoue, M., Padin, S., Wright, M.C.H., Zensus, A., Kus, A.J., Backer, D.C., Booth, R.S., Carlstrom, J.E., Dick-man, R. I., Emerson, D.T., Hirabayashi, H., Hodges, M.W., Kobayashi, H., Lamb, J., Moran, J.M., Morimoto, M., Plambeck, R.L., Predmore, C.R., Rönnäng, B., and Woody, D. 1992, A&A, 257, 31 Google Scholar
Colomer, F. 1993, “Subarcsecond Radio Astronomy” eds. Davies, and Booth, , in pressGoogle Scholar
Krichbaum, T. 1993, “Subarcsecond Radio Astronomy”, eds. Davies, and Booth, , in pressGoogle Scholar
Padin, S., Woody, D.P., Hodges, M.W., Rogers, A.E.E., Emerson, D.T., Jewel, P.R., Lamb, J., Perfetto, A., and Wright, M.C.H. 1990, AP.J., 360, L11 Google Scholar