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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| Published in: | Кинематика и физика небесных тел |
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| Date: | 2005 |
| Main Authors: | , , , , |
| Format: | Article |
| Language: | English |
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Головна астрономічна обсерваторія НАН України
2005
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| Online Access: | https://nasplib.isofts.kiev.ua/handle/123456789/79659 |
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| Journal Title: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Cite this: | 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| _version_ | 1862570704209182720 |
|---|---|
| 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. |
| 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. |
| collection | DSpace DC |
| container_title | 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.
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.
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| first_indexed | 2025-11-26T02:00:48Z |
| format | Article |
| fulltext | |
| id | nasplib_isofts_kiev_ua-123456789-79659 |
| institution | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| issn | 0233-7665 |
| language | English |
| last_indexed | 2025-11-26T02:00:48Z |
| publishDate | 2005 |
| publisher | Головна астрономічна обсерваторія НАН України |
| record_format | dspace |
| spelling | Lyubchik, Yu. Pavlenko, Ya.V. Jones, H.R.A. Tennyson, J. Pinfield, D. 2015-04-03T17:49:37Z 2015-04-03T17:49:37Z 2005 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 https://nasplib.isofts.kiev.ua/handle/123456789/79659 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. en Головна астрономічна обсерваторія НАН України Кинематика и физика небесных тел MS3: Physics of Stars and Galaxies Spectral energy distribution for GJ406 Article published earlier |
| spellingShingle | Spectral energy distribution for GJ406 Lyubchik, Yu. Pavlenko, Ya.V. Jones, H.R.A. Tennyson, J. Pinfield, D. MS3: Physics of Stars and Galaxies |
| title | 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_short | Spectral energy distribution for GJ406 |
| title_sort | spectral energy distribution for gj406 |
| topic | MS3: Physics of Stars and Galaxies |
| topic_facet | MS3: Physics of Stars and Galaxies |
| url | https://nasplib.isofts.kiev.ua/handle/123456789/79659 |
| work_keys_str_mv | AT lyubchikyu spectralenergydistributionforgj406 AT pavlenkoyav spectralenergydistributionforgj406 AT joneshra spectralenergydistributionforgj406 AT tennysonj spectralenergydistributionforgj406 AT pinfieldd spectralenergydistributionforgj406 |