Nature of X-ray emission from Nova Ophiuchi (H 1705-25)

Details Nature of X-ray emission from Nova Ophiuchi (H 1705-25) Nature of X-ray emission from Nova Ophiuchi (H 1705-25)

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....27..237k&link_type=abstract

Astrofizika (ISSN 0571-7132), vol. 27, Oct. 1987, p. 237-244. In Russian.

Astronomy and Astrophysics

Astronomy

Novae, Spectral Energy Distribution, Stellar Envelopes, X Ray Sources, Bremsstrahlung, Explosions, Flux Quantization, Photons, Shock Heating

Scientific paper

Explanation of the nature of the X-ray emission from the transient source nova Ophiuchi (H1705-25) based on the mechanism of thermal bremsstrahlung from a thin gas layer in a stellar envelope heated by a strong shock wave in the nova outburst has been given. An analytical expression for the observed spectrum that has time-dependent intensity and spectral distribution is obtained. The calculated spectra agree well with the observed data.

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