Hot components and circumstellar grains in M supergiant syncretic binaries
Copyright policy ) Richard H., Jr. Buss; Theodore P., Jr. Snow;
Hot components and circumstellar grains in M supergiant syncretic binaries
Ultraviolet and infrared spectra were obtained in order to study grains in cool star and hot star syncretic type binaries. Grains are found in only about half of the syncretic systems. The results suggest that grains have not formed in many syncretic systems because of ultraviolet radiation from the hot star. Circumstellar extinction could not be unambiguously detected in those systems with grains.
- University of Colorado Boulder United States
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selected citations
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These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
Citations provided by BIP!popularityPopularity provided by BIP!
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
Popularity provided by BIP! 6
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