Exploration of jet physics with some applications to SS 433

Details Exploration of jet physics with some applications to SS 433 Exploration of jet physics with some applications to SS 433

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..479k&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 479-482 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

3

Stellar Mass Ejection, Stellar Models, Supernova Remnants, X Ray Spectra, Emission Spectra, Plasma Jets, Stellar Activity, Stellar Spectra

Scientific paper

Theoretical X ray spectra in the model of homogenous jets and the model
of jets consisting of separated expanding spherical blobs were
calculated. Both models describe satisfactorily the continual component
(2 to 20 KeV) of X ray spectra of SS 433. Physical parameters of the
models were evaluated.

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