Spectral evidence for dust in late-type M dwarfs

Details Spectral evidence for dust in late-type M dwarfs Spectral evidence for dust in late-type M dwarfs

1997-02-13

arxiv.org/abs/astro-ph/9702108v1

Astronomy and Astrophysics

Astrophysics

9 pages, 5 postscript figs, ApJL accepted

Scientific paper

10.1086/310619

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).

Affiliated with

Also associated with

No associations

Rating

Spectral evidence for dust in late-type M dwarfs does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectral evidence for dust in late-type M dwarfs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral evidence for dust in late-type M dwarfs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-651821