Ammonia molecule and its applications in astrophysics

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Фізико-технічні та математичні науки
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Відділення фізики і астрономії
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Advances in Astronomy and Space Physics
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Advances in Astronomy and Space Physics, 2012, том 2
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Advances in Astronomy and Space Physics, 2012, вип. 1
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dc.contributor.author	Polinovskyi, G.
dc.contributor.author	Pavlenko, Ya.V.
dc.contributor.author	Tennyson, J.
dc.contributor.author	Yurchenko, S.N.
dc.contributor.author	Barber, R.J.
dc.date.accessioned	2017-06-04T18:28:55Z
dc.date.available	2017-06-04T18:28:55Z
dc.date.issued	2012
dc.identifier.citation	Ammonia molecule and its applications in astrophysics / G. Polinovskyi, Ya.V. Pavlenko, J. Tennyson, S.N. Yurchenko, R.J. Barber // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 17-19. — Бібліогр.: 17 назв. — англ.	uk_UA
dc.identifier.issn	2227-1481
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/119162
dc.description.abstract	Recently a new ammonia line list BYTe was reported comprising more than 1.1 billion transitions and designed for temperatures up to 1500 K. In this study we present an application of this line list for modelling spectra of cool star. We generated oscillator strengths of NH3 using BYTe for a frequency range of 1–5 µm and applied it for computing synthetic spectra of cool carbon giants using the WITA program. A possibility of detection of ammoniain spectra of cool carbon giants is discussed.	uk_UA
dc.description.sponsorship	We acknowledge funding by EU PF7 Marie Curie Initial Training Networks (ITN) ROPACS project (GA N 213646) and the ERC grant ERC-2010-AdG-267129 ExoMol.	uk_UA
dc.language.iso	en	uk_UA
dc.publisher	Головна астрономічна обсерваторія НАН України	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.title	Ammonia molecule and its applications in astrophysics	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA