Adaptive Optics Photometry and Astrometry of Binary Stars. II. A Multiplicity Survey of B Stars*

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Published 2007 January 9 © 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Lewis C. Roberts, Jr. et al 2007 AJ 133 545 DOI 10.1086/510335

1538-3881/133/2/545

Abstract

We carried out a search for companions to B stars using the adaptive optics system of the Advanced Electro-Optical System 3.6 m telescope. We observed 70 B stars in the I band, finding 16 companions, 10 of which are newly discovered companions. For each system with a detected companion we give its measured astrometry and differential magnitude. We then put the observation in context of the system's known multiplicity and provide a somewhat crude estimate of its spectral type based on the single differential magnitude measurement. The separations range from 0.2'' to 7.31'', and the differential magnitudes range from 1.41 ± 0.01 to 10.1 ± 0.5. Finally, we present a list of the null detections and discuss the implications of null detections of selected stars.

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Footnotes

  • Based on observations made at the Maui Space Surveillance System, operated by Detachment 15 of the US Air Force Research Laboratory's Directed Energy Directorate.

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10.1086/510335