Doppler-effect modulation of the observed radiation flux from ultracompact binary stars

Details Doppler-effect modulation of the observed radiation flux from ultracompact binary stars Doppler-effect modulation of the observed radiation flux from ultracompact binary stars

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...183l..21s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 183, no. 2, Sept. 1987, p. L21, L22.

Astronomy and Astrophysics

Astrophysics

5

Doppler Effect, Frequency Modulation, Radiant Flux Density, Stellar Mass Ejection, X Ray Binaries

Scientific paper

The observed radiation flux from ultra-short period binaries must be modulated due to Doppler effect. Different modulation amplitudes of integral flux should be seen depending on the geometry of the emitting object (a disc or a quasi-spherical source). When the source is observed in a narrow frequency band, Doppler modulation will be dependent on the shape of the spectrum also. The modulation will be more pronounced in the exponential tail of the spectrum.

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