HARD X-RAY-EMISSION FROM COLLIDING STELLA R WINDS

Authors
BYCHKOV KV SEIFINA EV
Citation
Kv. Bychkov et Ev. Seifina, HARD X-RAY-EMISSION FROM COLLIDING STELLA R WINDS, ASTRONOM ZH, 73(5), 1996, pp. 735-739
Citations number
12
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ASTRONOMICESKIJ ZURNAL
ISSN journal
00046299 → ACNP
Volume
73
Issue
5
Year of publication
1996
Pages
735 - 739
Database
ISI
SICI code
0004-6299(1996)73:5<735:HXFCSR>2.0.ZU;2-N
Abstract
A theoretical analysis of the emission from colliding stellar winds in binary systems is conducted. The fraction of emission from the region surrounding the ram point increases with energy of the emitted quanta ; therefore, it is most convenient to determine the flow parameters fr om observations in the hard X-ray range (E > 10 keV).