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Speckle Data in the New Bright Star Catalogue

Published online by Cambridge University Press:  12 April 2016

Wayne H. Warren Jr.  and
Dorrit Hoffleit
Wayne H. Warren Jr.
Affiliation:
Hughes STX Corp., NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
Dorrit Hoffleit
Affiliation:
Department of Astronomy, Yale University, Box 6666, New Haven CT, 06511, USA

Abstract

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The new fifth edition of the Bright Star Catalogue (BSC5) will include speckle interferometric data in specially allocated columns of the main catalog. Speckle observations have already been included for some 1,800 “bright” stars and more are expected from recent sources. In addition to the separations for resolved pairs, upper limits will be included for stars that have not been resolved. This paper describes how the speckle data have been incorporated into the catalog and gives examples of the new format.

Type
High Resolution At Visual Wavelengths
Information
International Astronomical Union Colloquium , Volume 135: Complementary Approaches to Double and Multiple Star Research , 1992 , pp. 580 - 582
Copyright
Copyright © Astronomical Society of the Pacific 1992

References

Hoffleit, D. (with the collaboration of Jaschek, C.) 1982, The Bright Star Catalogue, 4th revised edition (New Haven, Yale Univ. Observatory)Google Scholar
McAlister, H.A. & Hartkopf, W.I. 1988, Second Catalog of Interferometric Measurements of Binary Stars, CHARA Contrib. No. 2 (Atlanta, Center for Higher Angular Resolution Astronomy, Georgia State Univ.)Google Scholar