Spectral energy distribution for GJ406

We present results of modelling the bulk of the spectral energy distribution (0.45–5 μm) for GJ406 (M6V). Synthetic spectra were calculated using the NextGen model atmospheres of Hauschildt et al. [6] and the incorporate line lists for H2O, TiO, CrH, FeH, CO, MgH molecules as well as the VALD line l...

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Дата:2005
Автори: Lyubchik, Yu., Pavlenko, Ya.V., Jones, H.R.A., Tennyson, J., Pinfield, D.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2005
Назва видання:Кинематика и физика небесных тел
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Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/79659
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Spectral energy distribution for GJ406 / Yu. Lyubchik, Ya.V. Pavlenko, H.R.A. Jones, J. Tennyson, D. Pinfield // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 279-282. — Бібліогр.: 14 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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spelling irk-123456789-796592015-04-04T03:01:47Z Spectral energy distribution for GJ406 Lyubchik, Yu. Pavlenko, Ya.V. Jones, H.R.A. Tennyson, J. Pinfield, D. MS3: Physics of Stars and Galaxies We present results of modelling the bulk of the spectral energy distribution (0.45–5 μm) for GJ406 (M6V). Synthetic spectra were calculated using the NextGen model atmospheres of Hauschildt et al. [6] and the incorporate line lists for H2O, TiO, CrH, FeH, CO, MgH molecules as well as the VALD line list of atomic lines. The computed water partition function is in a good agreement with the one obtained by Vidler & Tennyson [14]. A comparison of synthetic and observed spectra gives Teff = 2900 ± 100 K for this late M-dwarf. The William Herschel Telescope and United Kingdom Infrared Telescope are operated for the Particle Physics and Astronomy Research Council (PPARC). ISO is an ESA project with the participation of ISAS and NASA funded from member states. HST is a NASA project funded in part by ESA. This work was partially supported by a PPARC visitors grants from PPARC and the Royal Society. YP’s studies are partially supported by a Small Research Grant from American Astronomical Society. This research has made with the use of the SIMBAD database, operated at CDS, Strasbourg, France. 2005 Article Spectral energy distribution for GJ406 / Yu. Lyubchik, Ya.V. Pavlenko, H.R.A. Jones, J. Tennyson, D. Pinfield // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 279-282. — Бібліогр.: 14 назв. — англ. 0233-7665 http://dspace.nbuv.gov.ua/handle/123456789/79659 en Кинематика и физика небесных тел Головна астрономічна обсерваторія НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
topic MS3: Physics of Stars and Galaxies
MS3: Physics of Stars and Galaxies
spellingShingle MS3: Physics of Stars and Galaxies
MS3: Physics of Stars and Galaxies
Lyubchik, Yu.
Pavlenko, Ya.V.
Jones, H.R.A.
Tennyson, J.
Pinfield, D.
Spectral energy distribution for GJ406
Кинематика и физика небесных тел
description We present results of modelling the bulk of the spectral energy distribution (0.45–5 μm) for GJ406 (M6V). Synthetic spectra were calculated using the NextGen model atmospheres of Hauschildt et al. [6] and the incorporate line lists for H2O, TiO, CrH, FeH, CO, MgH molecules as well as the VALD line list of atomic lines. The computed water partition function is in a good agreement with the one obtained by Vidler & Tennyson [14]. A comparison of synthetic and observed spectra gives Teff = 2900 ± 100 K for this late M-dwarf.
format Article
author Lyubchik, Yu.
Pavlenko, Ya.V.
Jones, H.R.A.
Tennyson, J.
Pinfield, D.
author_facet Lyubchik, Yu.
Pavlenko, Ya.V.
Jones, H.R.A.
Tennyson, J.
Pinfield, D.
author_sort Lyubchik, Yu.
title Spectral energy distribution for GJ406
title_short Spectral energy distribution for GJ406
title_full Spectral energy distribution for GJ406
title_fullStr Spectral energy distribution for GJ406
title_full_unstemmed Spectral energy distribution for GJ406
title_sort spectral energy distribution for gj406
publisher Головна астрономічна обсерваторія НАН України
publishDate 2005
topic_facet MS3: Physics of Stars and Galaxies
url http://dspace.nbuv.gov.ua/handle/123456789/79659
citation_txt Spectral energy distribution for GJ406 / Yu. Lyubchik, Ya.V. Pavlenko, H.R.A. Jones, J. Tennyson, D. Pinfield // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 279-282. — Бібліогр.: 14 назв. — англ.
series Кинематика и физика небесных тел
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AT pavlenkoyav spectralenergydistributionforgj406
AT joneshra spectralenergydistributionforgj406
AT tennysonj spectralenergydistributionforgj406
AT pinfieldd spectralenergydistributionforgj406
first_indexed 2023-10-18T19:19:12Z
last_indexed 2023-10-18T19:19:12Z
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