Discovery of SiO Masers in the "Water Fountain" Source IRAS 16552-3050
文献类型：期刊论文
| 作者 | Amada, K.11; Imai, H.9,10,11; Hamae, Y.8; Nakashima, K.8; Shum, K. Y.8; Tafoya, D.7; Uscanga, L.6; Gomez, J. F.5; Orosz, G.3,4 ; Burns, R. A.1,2
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| 刊名 | ASTRONOMICAL JOURNAL
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| 出版日期 | 2022-02-01 |
| 卷号 | 163期号:2页码:5 |
| ISSN号 | 0004-6256 |
| DOI | 10.3847/1538-3881/ac3fb6 |
| 通讯作者 | Amada, K.(k0501862@kadai.jp) |
| 英文摘要 | In this paper, we report new detections of SiO v = 1 and v = 2 J = 1 -> 0 masers in the "water fountain" source IRAS 16552-3050, which was observed with the Nobeyama 45 m telescope during 2021 March-April. Water fountains are evolved stars whose H2O maser spectra trace high-velocity outflows of >100 km s(-1). This is the second known case of SiO masers in a water fountain, after their prototypical source, W 43A. These SiO masers should shed light on the evolutionary status of this category of evolved stars, which are likely to be at the end of the asymptotic giant branch phase, when the star exhibits the most copious stellar mass loss, followed by development of the complicated morphologies of planetary nebulae. The origin of a large (up to 25 km s(-1)) velocity offset of the SiO masers with respect to the systemic velocity derived from the spectrum of CO J = 2 -> 1 line is discussed here. |
| WOS关键词 | POSTASYMPTOTIC GIANT BRANCH ; POST-AGB STARS ; PLANETARY-NEBULAE ; H2O MASERS ; W43A |
| 资助项目 | ALMA[2018.1.00250.S] ; National Aeronautics and Space Administration ; JSPS KAKENHI[JP 16H02167] ; State Agency for Research (AEI) of the Spanish MCIU[PID2020114461GB-I00] ; Center of Excellence Severo Ochoa award[SEV2017-0709] |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:000746170500001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | ALMA ; National Aeronautics and Space Administration ; JSPS KAKENHI ; State Agency for Research (AEI) of the Spanish MCIU ; Center of Excellence Severo Ochoa award |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/4444]  |
| 专题 | 星系宇宙学研究团组 |
| 通讯作者 | Amada, K. |
| 作者单位 | 1.Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea 2.Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan 3.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 4.Univ Tasmania, Sch Nat Sci, Private Bag 37, Hobart, Tas 7001, Australia 5.CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, E-18008 Granada, Spain 6.Univ Guanajuato, Dept Astron, AP 144, Guanajuato 36000, Gto, Mexico 7.Chalmers Univ Technol, Onsala Space Observ, Dept Space Earth & Environm, SE-43992 Onsala, Sweden 8.Kagoshima Univ, Fac Sci, Dept Phys & Astron, 1-21-35 Korimoto, Kagoshima 8900065, Japan 9.Kagoshima Univ, Ctr Gen Educ, Inst Comprehens Educ, 1-21-30 Korimoto, Kagoshima 8900065, Japan 10.Kagoshima Univ, Amanogawa Galaxy Astron Res Ctr, Grad Sch Sci & Engn, 1-21-35 Korimoto, Kagoshima 8900065, Japan |
| 推荐引用方式 GB/T 7714 | Amada, K.,Imai, H.,Hamae, Y.,et al. Discovery of SiO Masers in the "Water Fountain" Source IRAS 16552-3050[J]. ASTRONOMICAL JOURNAL,2022,163(2):5. |
| APA | Amada, K..,Imai, H..,Hamae, Y..,Nakashima, K..,Shum, K. Y..,...&Burns, R. A..(2022).Discovery of SiO Masers in the "Water Fountain" Source IRAS 16552-3050.ASTRONOMICAL JOURNAL,163(2),5. |
| MLA | Amada, K.,et al."Discovery of SiO Masers in the "Water Fountain" Source IRAS 16552-3050".ASTRONOMICAL JOURNAL 163.2(2022):5. |
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