A jet model for a very high state of GX 339 - 4

Details A jet model for a very high state of GX 339 - 4 A jet model for a very high state of GX 339 - 4

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...374..741m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 374, June 20, 1991, p. 741-743.

Astronomy and Astrophysics

Astronomy

27

Black Holes (Astronomy), Compton Effect, Stellar Models, X Ray Binaries, Energy Spectra, Photons, Stellar Luminosity, Thomson Scattering

Scientific paper

A jet model is proposed which explain results derived by Ginga observation of GX 339 - 4 in its very high state. Specifically, the model can explain: (1) the possible existence of large Compton clouds of 1-billion-cm size; (2) the independent change of the soft and hard components in the long term; (3) the rapid variability of the hard tail component in the short term; and (4) the possible existence of absorbing matter around the compact star.

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