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- W1585362010 abstract "The atmospheric structure of the dwarf M-stars which is especially important to the general field of stellar chromospheres and coronae was investigated. The M-dwarf stars constitute a class of objects for which the discrepancy between the predictions of the acoustic wave chromospheric/coronal heating hypothesis and the observations is most vivid. It is assumed that they represent a class of stars where alternative atmospheric heating mechanisms, presumably magnetically related, are most clearly manifested. Ascertainment of the validity of a hypothesis to account for the origin of the chromospheric and transition region line emission in M-dwarf stars is proposed." @default.
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- W1585362010 date "1982-02-01" @default.
- W1585362010 modified "2023-09-22" @default.
- W1585362010 title "A heating mechanism for the chromospheres of M dwarf stars" @default.
- W1585362010 hasPublicationYear "1982" @default.
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