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- W2040471846 abstract "Infrared photometry of S Per, $mu$ Cep, and HD 11979 reveals that these stars have substantially larger flux excesses at 33 $mu$ than do $alpha$ Ori and o Cet. These prominent excesses may be attributable to a distinct lattice band in circumstellar dust grains composed of silicates such as $gamma$-Ca$sub 2$SiO$sub 4$, Fe$sub 2$SiO$sub 4$, or Mn$sub 2$SiO$sub 4$. The observations show that the abundance of this silicate material varies dramatically from one star to another among the class of M stars. (AIP)" @default.
- W2040471846 created "2016-06-24" @default.
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- W2040471846 date "1975-10-01" @default.
- W2040471846 modified "2023-09-24" @default.
- W2040471846 title "Possible identification of a circumstellar 33-micron silicate emission band in cool-star spectra" @default.
- W2040471846 doi "https://doi.org/10.1086/181947" @default.
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