| dc.contributor.author | Jones, H.R.A. | |
| dc.contributor.author | Tsuji, Takashi | |
| dc.date.accessioned | 2012-01-17T18:01:09Z | |
| dc.date.available | 2012-01-17T18:01:09Z | |
| dc.date.issued | 1997-02-13 | |
| dc.identifier.citation | Jones , H R A & Tsuji , T 1997 , ' Spectral evidence for dust in late-type M dwarfs ' , Astrophysical Journal Letters , vol. 480 , L39 . https://doi.org/10.1086/310619 | |
| dc.identifier.issn | 2041-8213 | |
| dc.identifier.other | ArXiv: http://arxiv.org/abs/astro-ph/9702108v1 | |
| dc.identifier.uri | http://hdl.handle.net/2299/7676 | |
| dc.description | 9 pages, 5 postscript figs, ApJL accepted | |
| dc.description.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). | en |
| dc.format.extent | 183630 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Astrophysical Journal Letters | |
| dc.subject | astro-ph | |
| dc.title | Spectral evidence for dust in late-type M dwarfs | en |
| dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
| dc.contributor.institution | School of Physics, Engineering & Computer Science | |
| dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Centre of Data Innovation Research | |
| dc.description.status | Peer reviewed | |
| rioxxterms.versionofrecord | 10.1086/310619 | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
