Published in

American Astronomical Society, Astronomical Journal, 2(136), p. 554-565, 2008

DOI: 10.1088/0004-6256/136/2/554

Links

Tools

Export citation

Search in Google Scholar

Adaptive Optics Photometry and Astrometry of Binary Stars. III. A Faint Companion Search of O-Star Systems

Journal article published in 2008 by Nils H. Turner, Theo A. ten Brummelaar, Theo A. ten Brummelaar, Lewis C. Roberts ORCID, Brian D. Mason, William I. Hartkopf, Douglas R. Gies
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

Full text: Download

Red circle
Preprint: archiving forbidden
Red circle
Postprint: archiving forbidden
Green circle
Published version: archiving allowed
Upload
Policy details
Data provided by SHERPA/RoMEO

Abstract

We present the results of an adaptive optics survey for faint companions among Galactic O-type star systems (V < 8) using the Advanced Electro-Optical System (AEOS) 3.6-meter telescope on Haleakala. We surveyed these O star systems in I-band, typically being able to detect a companion with a magnitude difference of about 6 in the projected separation range of 0.5 to 1.0 arcseconds, and of about 9.5 in the range of 1.0 to 5.0 arcseconds. In the course of the survey, we discovered 40 new companions among 31 of the 116 objects examined and made astrometric and differential magnitude measurements of 24 additional known pairs, several of them being confirmation detections. We present new astrometric orbits for two binaries, BU 1032AB (WDS 05387-0236; sig Ori AB) and SEE 322 (WDS 17158-3344; HD 155889AB). We lack magnitude differences for other filter bands, so it is difficult to determine physical from line-of-sight companions, but we present empirical arguments for the limiting magnitude difference where field contamination is significant. Comment: 34 pages, 7 figures, 6 tables, accepted for publication in the Astronomical Journal