Variable dust formation by the double-line spectroscopic binary WR 70 (HD 137603, WC9vd+B0I)

Author:

Williams Peredur M.,van der Hucht Karel A.,Marang Fred

Abstract

Infrared photometry of the WC9vd+B0I spectroscopic binary WR 70 over two decades shows variable dust emission. The variations are relatively slow and show evidence for an underlying process with a period P = 1045 ± 60 d, together with modulation on shorter and longer time-scales.

Publisher

Cambridge University Press (CUP)

Reference6 articles.

1. Golombek D.A. 1983, Estudio Espectrografico de Una Estrella Supergiante con Líneas de Emisión, PhD thesis, Universidad de Buenos Aires, Argentina.

2. Infrared Observations of Southern WC9 Stars and He 2-113

3. Dhillon V.S. , Privett G.J. 1997, period time-series analysis package, Starlink User Note 167.5, Rutherford Appleton Laboratory.

4. Revised Wolf-Rayet Binary Orbits and New Binaries

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