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dc.contributor.author |
Pavlenko, Ya.V. |
|
dc.date.accessioned |
2015-04-03T17:33:46Z |
|
dc.date.available |
2015-04-03T17:33:46Z |
|
dc.date.issued |
2005 |
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dc.identifier.citation |
Ultracool dwarfs / Ya.V. Pavlenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 244-249. — Бібліогр.: 44 назв. — англ. |
uk_UA |
dc.identifier.issn |
0233-7665 |
|
dc.identifier.uri |
http://dspace.nbuv.gov.ua/handle/123456789/79651 |
|
dc.description.abstract |
We present results of modelling of spectra of M-, L-, T-dwarfs. Theoretical spectra are fitted to observed spectra to study the main parameters of the low-mass objects beyond the bottom of the Main Sequence. Application of the “lithium” and “deuterium” tests for assessment of ultra-cool dwarfs is discussed. |
uk_UA |
dc.description.sponsorship |
I thank Maria Rosa Zapatero Osorio (LAEFF, Spain) for her highlighted and helpful comments. I am grateful to my collaborators and co-authors Hugh R. A. Jones (Univ. of Hertfordshire, UK), Rafael Rebolo, Mart´ın Eduardo, V´ıctor J. S. B´ejar (IAC, Spain) for their contribution. My investigations were supported by a Small Research Grant of AAS and a Royal Society travel grant as well as travel grants from Liverpool University (UK). |
uk_UA |
dc.language.iso |
en |
uk_UA |
dc.publisher |
Головна астрономічна обсерваторія НАН України |
uk_UA |
dc.relation.ispartof |
Кинематика и физика небесных тел |
|
dc.subject |
MS3: Physics of Stars and Galaxies |
uk_UA |
dc.title |
Ultracool dwarfs |
uk_UA |
dc.type |
Article |
uk_UA |
dc.status |
published earlier |
uk_UA |
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