The environs of the massive runaway star BD+43^o 3654

Details The environs of the massive runaway star BD+43^o 3654 The environs of the massive runaway star BD+43^o 3654

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010rmxac..38...61p&link_type=abstract

The Interferometric View on Hot Stars (Eds. Th. Rivinius & M. Curé) Revista Mexicana de Astronomía y Astrofísica (Serie de Confe

Astronomy and Astrophysics

Astronomy

1

H Ii Regions, Ism: Jets And Outflows, Stars: Mass Loss, Stars: Pre-Main Sequence

Scientific paper

The very massive runaway star BD+43° 3654 (O4 If) seems to be related with a bow shock detected by the MSX mission, that would be the result of the interaction of the strong stellar wind with the ambient matter. Shock-accelerated electrons will cool through synchrotron radiation producing a non-thermal radio source, yet never detected in such scenario. While new Very Large Array observations are carried out, we have examined archive data and present here the findings.

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