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The Southern Hemisphere VLBI Experiment (Sheve)

  • R.A. Preston (a1), D.L. Jauncey (a2), A. Tsioumis (a3), D.L. Meier (a1), L.J. Skjerve (a1), J. Ables (a2), R. Batchelor (a2), J. Faulkner (a1), P.M. Hamilton (a4), R. Haynes (a2), B. Johnson (a5), A. Louie (a1), P. McCulloch (a4), G. Moorey (a2), D.D. Morabito (a1), G. Nicolson (a6), A.E. Niell (a1), J.G. Robertson (a7), G.W.R. Royle (a8), M.A. Slade (a1), O.B. Slee (a2), A. Watkinson (a3), A.E. Wehrle (a1) and A. Wright (a2)...

Extract

The Southern Hemisphere VLBI Experiment (or SHEVE) was a joint US-Australian-South African venture with both astronomy and geodesy goals. The principle astronomy goal was to make models or maps of the following sources: at 2.3 GHz (with six antennas and 9 usable baselines) – Centaurus A (the nearest active galaxy), Circinus X-1 (a flaring binary), the VELA pulsar, and 26 other active galactic nuclei and quasars; at 8.4 GHz (only one baseline) – Centaurus A and the galactic center.

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Copyright

References

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Preston, et al. 1983, Ap. J. (Letters), 266, 93.
Phillips, and Mutel, 1981, Ap. J., 244, 19.
Gubbay, J. S. et al. 1971, A. J., 76, 965.
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Proceedings of the International Astronomical Union
  • ISSN: -
  • EISSN: 0074-1809
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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