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Radio light-curve for WR 146 (HM19-3, WC6+O8.5), a colliding wind binary∗
Published online by Cambridge University Press: 25 May 2016
Abstract
We report preliminary results of monitoring the flux from the Wolf-Rayet object WR 146 with the Westerbork Synthesis Radio Telescope at 21 cm since 1989. We find the average flux density slowly rising in the period 1989–1997, with evidence of shorter time-scale variability.
- Type
- Part 3. Interaction of Wolf-Rayet stars and other hot massive stars with their environment: colliding winds and ring nebulae
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- Copyright © Astronomical Society of the Pacific 1999