Mass flow in close binaries - Results of optical and ultraviolet observations

Details Mass flow in close binaries - Results of optical and ultraviolet observations Mass flow in close binaries - Results of optical and ultraviolet observations

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979s%26w....18...49r&link_type=abstract

Sterne und Weltraum, vol. 18, Feb. 1979, p. 49-54. In German.

Astronomy and Astrophysics

Astronomy

Binary Stars, Mass Flow, Stellar Envelopes, Ultraviolet Astronomy, Visual Observation, Astronomical Photometry, Centaurus Constellation, Cepheid Variables, Cygnus Constellation, Iue, Oao 3, Stellar Models, Stellar Spectrophotometry

Scientific paper

Observational data provide information regarding mass flow in close binaries. Data about origin, condition, and development of circumstellar matter can also be obtained. The investigations are based on an evaluation and correlation of photometric observations and simultaneously made photoelectric and spectrographic observations in the visible spectral range and, in addition, also on satellite observations in the ultraviolet range. Supplementary information concerning the mass flow in close binaries is obtained on the basis of observations related to the X-ray, infrared, and radio range. Suitable theoretical models are employed to interpret the observational data.

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