Radio study on the mass loss bi-stability jump

Details Radio study on the mass loss bi-stability jump Radio study on the mass loss bi-stability jump

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..33...65b&link_type=abstract

Massive Stars: Fundamental Parameters and Circumstellar Interactions (Eds. P. Benaglia, G. L. Bosch, & C. E. Cappa) Revista Mexi

Astronomy and Astrophysics

Astronomy

2

Radio Continuum: Stars, Stars: Early-Type, Stars: Mass Loss, Stars: Winds, Outflows

Scientific paper

By means of radio continuum observations of 29 stars with spectral types O8-B3 we searched for evidence of the existence of a bi-stability jump in stellar mass loss around T_{eff} ≈ 21 kK. Although there are quantitative discrepancies, the qualitative behaviour of the wind efficiency with effective temperature appears to be in line with theoretical predictions. Observations of new cases are fundamental to confirm these results.

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