Nature of OH maser and SiO thermal emission towards carbon star: IRAS 05373-0810 (V1187 Ori) | |
Szczerba, R1; Chen PS(陈培生)2![]() | |
发表期刊 | ASTRONOMY & ASTROPHYSICS
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2002-01 | |
卷号 | 381期号:2页码:491-499 |
DOI | 10.1051/0004-6361:20011518 |
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 |
ISSN | 0004-6361 |
URL | 查看原文 |
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 |
引用统计 | |
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 |
推荐引用方式 GB/T 7714 | 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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Nature of OH maser a(209KB) | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
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