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Nature of OH maser and SiO thermal emission towards carbon star: IRAS 05373-0810 (V1187 Ori)
Szczerba, R1; Chen PS(陈培生)2; Szymczak, M3; Omont, A4; Szczerba, R (reprint author), Nicholas Copernicus Astron Ctr, Rabianska 8, PL-87100 Torun, Poland.
发表期刊ASTRONOMY & ASTROPHYSICS
2002-01
卷号381期号:2页码:491-499
DOI10.1051/0004-6361:20011518
产权排序第2完成单位
收录类别SCI
关键词Individual : Iras05373-0810 Stars : Agb And post-Agb Carbon Ism : Dust Extinction
摘要We present observational evidence that IRAS 05373-0810 is a genuine carbon star with an ISO SWS spectrum closely resembling that of RScl. Modelling of the spectral energy distribution of IRAS05373-0810 ;suggests that the star has luminosity of order of 8000 L(.) and loses mass at a rate of about 2-3 x 10(-7) M(.) yr(-1). The detected OH maser emission at 1612, 1665 and 1667 MHz arid SiO thermal emission at 86.85 GHz towards IRAS05373-0810 is not associated with this source. The available observations imply that these lines, typical for O-rich sources, come from the molecular cloud L 1641 in the Orion star forming region (OH) and. very likely, from the NGC 2149 molecular complex (SiO).
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0004-6361
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归档日期2002-05-17
WOS记录号WOS:000173343100015
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]CIRCUMSTELLAR DUST SHELLS ; SILICATE DUST ; INFRARED OBSERVATIONS ; STELLAR POPULATION ; MOLECULAR CLOUDS ; IRAS SOURCES ; OH/IR STARS ; LRS SPECTRA ; V778 CYGNI ; DARK CLOUD
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被引频次:6[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/4148
专题其他
通讯作者Szczerba, R (reprint author), Nicholas Copernicus Astron Ctr, Rabianska 8, PL-87100 Torun, Poland.
作者单位1.N. Copernicus Astronomical Center, Rabianska 8, 87-100 Torun, Poland
2.Yunnan Astronomical Observatory, National Observatory, CAS, Kunming 650011, PR China
3.Torun Centre for Astronomy, Nicolaus Copernicus University, Gagarina 11, 87-100 Torun, Poland
4.Institut d'Astrophysique, 98bis boulevard Arago, 75014 Paris, France
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Szczerba, R,Chen PS,Szymczak, M,et al. Nature of OH maser and SiO thermal emission towards carbon star: IRAS 05373-0810 (V1187 Ori)[J]. ASTRONOMY & ASTROPHYSICS,2002,381(2):491-499.
APA Szczerba, R,Chen PS,Szymczak, M,Omont, A,&Szczerba, R .(2002).Nature of OH maser and SiO thermal emission towards carbon star: IRAS 05373-0810 (V1187 Ori).ASTRONOMY & ASTROPHYSICS,381(2),491-499.
MLA Szczerba, R,et al."Nature of OH maser and SiO thermal emission towards carbon star: IRAS 05373-0810 (V1187 Ori)".ASTRONOMY & ASTROPHYSICS 381.2(2002):491-499.
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