Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-06-08
Astronomy and Astrophysics
Astrophysics
Accepted for publication in PASP July 2007 issue
Scientific paper
10.1086/520707
We present new results from a radial velocity study of six bright OB stars with little or no prior measurements. One of these, HD 45314, may be a long-period binary, but the velocity variations of this Be star may be related to changes in its circumstellar disk. Significant velocity variations were also found for HD 60848 (possibly related to nonradial pulsations) and HD 61827 (related to wind variations). The other three targets, HD 46150, HD 54879, and HD 206183, are constant velocity objects, but we note that HD 54879 has H$\alpha$ emission that may originate from a binary companion. We illustrate the average red spectrum of each target.
Baines Ellyn K.
Barai Paramita
Boyajian Tabetha S.
Gies Douglas R.
Grundstrom Erika D.
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