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- W2014382783 abstract "The observed infrared emission from R CrB and RY Sgr can be explained as due to thermal emission from the shell of dust grains surrounding these stars. We have calculated the emission spectmm of the dust shell as a function of the visual magnitude and also the expected flux of the star as a function of the optical depth of the dust shelL The question of the condensation of graphite particles in these stars is briefly discussed. Key words: infrared emission - dust grains - carbon stars" @default.
- W2014382783 created "2016-06-24" @default.
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- W2014382783 date "1972-02-01" @default.
- W2014382783 modified "2023-09-26" @default.
- W2014382783 title "Dust Model for R Coronae Borealis and RY Sagittarii" @default.
- W2014382783 doi "https://doi.org/10.1086/129247" @default.
- W2014382783 hasPublicationYear "1972" @default.
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