Radiative Acceleration of Heavy Ions in the Winds of O-B Stars

Details Radiative Acceleration of Heavy Ions in the Winds of O-B Stars Radiative Acceleration of Heavy Ions in the Winds of O-B Stars

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.215v&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

It is shown, that the radiation pressure force can accelerate the ions with the strong resonance lines in the hot-star stellar winds. The acceleration up to several MeV energy value is possible in the intershock layers of the shock-structured stellar winds. Possible nuclear reactions due to acceleration of the CIV and SiIV ions are considered and the relative problems are discussed.

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