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Spectral evidence for dust in late-type M dwarfs | | Hugh R. A. Jones
; Takashi Tsuji
; | | Date: |
13 Feb 1997 | | Subject: | astro-ph | | Abstract: | We have found a dramatic change in the spectra of late-type M dwarfs at wavelengths shorter than 0.75 microns. Comparisons with synthetic spectra illustrate that this change is well explained by the presence of dust. It thus seems that a substantial part of the long-standing discrepancies between late-type M dwarf models and observations arises from dust as recently proposed by Tsuji, Ohnaka and Aoki (1996a). | | Source: | arXiv, astro-ph/9702108 | | Services: | Forum | Review | PDF | Favorites | |
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