The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope | |
Scicluna, P3,4; Kemper, F3,5; McDonald, I6,7; Srinivasan, S3,8; Trejo, A3; Wallström, S H J3,9; Wouterloot, J G A1; Cami, J10,11,12; Greaves, J13; He JH(何金华)14,15,16 | |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
2022-04-04 | |
卷号 | 512期号:1页码:1091-1110 |
关键词 | catalogues surveys stars: AGB and post-AGB stars: mass-loss stars: winds outflows |
ISSN号 | 0035-8711 |
DOI | 10.1093/mnras/stab2860 |
产权排序 | 第13完成单位 |
文献子类 | Article |
英文摘要 | The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of similar to 850 Galactic evolved stars within 3 kpc at (sub-)mm wavelengths, observed in the CO J = (2-1) and (3-2) rotational lines, and the sub-mm continuum, using the James Clark Maxwell Telescope and Atacama Pathfinder Experiment. NESS consists of five tiers, based on distances and dust-production rate (DPR). We define a new metric for estimating the distances to evolved stars and compare its results to Gaia EDR3. Replicating other studies, the most-evolved, highly enshrouded objects in the Galactic Plane dominate the dust returned by our sources, and we initially estimate a total DPR of 4.7 x 10(-5) M-circle dot yr(-1) from our sample. Our sub-mm fluxes are systematically higher and spectral indices are typically shallower than dust models typically predict. The 450/850 $\mu$m spectral indices are consistent with the blackbody Rayleigh-Jeans regime, suggesting a large fraction of evolved stars have unexpectedly large envelopes of cold dust. |
学科主题 | 天文学 ; 恒星与银河系 ; 恒星形成与演化 |
URL标识 | 查看原文 |
出版地 | GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND |
资助项目 | National Key R&D Programme of China[2017YFA0402700] ; Science and Technology Facilities Council of the United KingdomUK Research & Innovation (UKRI)Science & Technology Facilities Council (STFC) ; Ministry of Science and Technology of TaiwanMinistry of Science and Technology, Taiwan[MOST1042628-M-001-004-MY3] ; Ministry of Science and Technology of TaiwanMinistry of Science and Technology, Taiwan[MOST107-2119-M-001-031-MY3] ; Ministry of Science and Technology of TaiwanMinistry of Science and Technology, Taiwan[MOST109-2112-M-001-036-MY3] ; Academia SinicaAcademia Sinica - Taiwan[AS-IA-106-M03] ; UK Science and Technology Facilities CouncilUK Research & Innovation (UKRI)Science & Technology Facilities Council (STFC)[ST/L00768/1] ; UK Science and Technology Facilities CouncilUK Research & Innovation (UKRI)Science & Technology Facilities Council (STFC)[ST/P000649/1] ; UK Science and Technology Facility Council[ST/P000649/1] ; UK Science and Technology Facility Council[ST/L000768/1] ; UNAM-PAPIIT Programme[IA104820] ; Research Foundation Flanders (FWO)FWO[1285221N] ; ERCEuropean Research Council (ERC)European Commission[646758 AEROSOL] ; EU's Horizon 2020 programme under the Marie Sklodowska-Curie grant[665593] ; Daiwa Anglo-Japan Foundation ; Great Britain Sasakawa Foundation ; European Research Council (ERC)European Research Council (ERC)European Commission[ERC-2014-CoG-647939] ; STFC Ernest Rutherford fellowshipUK Research & Innovation (UKRI)Science & Technology Facilities Council (STFC)[ST/L003597/1] ; Natural Sciences and Engineering Research Council (NSERC)Natural Sciences and Engineering Research Council of Canada (NSERC) ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11873086] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[U1631237] ; Yunnan Province of China[2017HC018] ; NASANational Aeronautics & Space Administration (NASA)[80GSFC17M0002] ; National Research Foundation of Korea (NRF) - Korea government (MIST)National Research Foundation of Korea[2021R1A2C1008928] ; Chinese Academy of Sciences (CAS)Chinese Academy of Sciences ; [M17BL002] |
WOS关键词 | MASS-LOSS RATES ; PERIOD-LUMINOSITY RELATION ; CIRCUMSTELLAR CO EMISSION ; CARBON-MONOXIDE EMISSION ; REVISED AFGL CATALOGS ; LOW-TEMPERATURE MIR ; GIANT BRANCH STARS ; AGB STARS ; TP-AGB ; ABSORPTION-COEFFICIENT |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | OXFORD UNIV PRESS |
WOS记录号 | WOS:000778666900001 |
资助机构 | National Key R&D Programme of China[2017YFA0402700] ; Science and Technology Facilities Council of the United KingdomUK Research & Innovation (UKRI)Science & Technology Facilities Council (STFC) ; Ministry of Science and Technology of TaiwanMinistry of Science and Technology, Taiwan[MOST1042628-M-001-004-MY3, MOST107-2119-M-001-031-MY3, MOST109-2112-M-001-036-MY3] ; Academia SinicaAcademia Sinica - Taiwan[AS-IA-106-M03] ; UK Science and Technology Facilities CouncilUK Research & Innovation (UKRI)Science & Technology Facilities Council (STFC)[ST/L00768/1, ST/P000649/1] ; UK Science and Technology Facility Council[ST/P000649/1, ST/L000768/1] ; UNAM-PAPIIT Programme[IA104820] ; Research Foundation Flanders (FWO)FWO[1285221N] ; ERCEuropean Research Council (ERC)European Commission[646758 AEROSOL] ; EU's Horizon 2020 programme under the Marie Sklodowska-Curie grant[665593] ; Daiwa Anglo-Japan Foundation ; Great Britain Sasakawa Foundation ; European Research Council (ERC)European Research Council (ERC)European Commission[ERC-2014-CoG-647939] ; STFC Ernest Rutherford fellowshipUK Research & Innovation (UKRI)Science & Technology Facilities Council (STFC)[ST/L003597/1] ; Natural Sciences and Engineering Research Council (NSERC)Natural Sciences and Engineering Research Council of Canada (NSERC) ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11873086, U1631237] ; Yunnan Province of China[2017HC018] ; NASANational Aeronautics & Space Administration (NASA)[80GSFC17M0002] ; National Research Foundation of Korea (NRF) - Korea government (MIST)National Research Foundation of Korea[2021R1A2C1008928] ; Chinese Academy of Sciences (CAS)Chinese Academy of Sciences ; [M17BL002] |
内容类型 | 期刊论文 |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/25037] |
专题 | 云南天文台_大样本恒星演化研究组 |
通讯作者 | Scicluna, P |
作者单位 | 1.East Asian Observatory (JCMT), 660 N. A‘ohoku Place, Hilo, HI 96720, USA; 2.Department of Astronomy and Space Science, CHUNGBUK NATIONAL UNIVERSITY, Cheongju-City, 28644, Republic of Korea; 3.Institute of Astronomy and Astrophysics, Academia Sinica, 11F of AS/NTU Astronomy-Mathematics Building, No. 1, Section 4, Roosevelt Rd, Taipei 10617, Taiwan; 4.European Southern Observatory, Alonso de Cordova 3107, Santiago RM, Chile; 5.European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching b. München, Germany; 6.Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, School of Natural Sciences, University of Manchester, M13 9PL Manchester, UK; 7.Department of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK; 8.Instituto de Radioastronomía y Astrofísica, UNAM. Apdo. Postal 72-3 (Xangari), Morelia, Michoacán 58089, Michoacán, Mexico; 9.Institute of Astronomy, KU Leuven, Celestijnenlaan 200D bus 2401, B-3001 Leuven, Belgium; 10.Department of Physics and Astronomy, University of Western Ontario, London, ON N6A 3K7, Canada; |
推荐引用方式 GB/T 7714 | Scicluna, P,Kemper, F,McDonald, I,et al. The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2022,512(1):1091-1110. |
APA | Scicluna, P.,Kemper, F.,McDonald, I.,Srinivasan, S.,Trejo, A.,...&Zijlstra, A A.(2022).The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,512(1),1091-1110. |
MLA | Scicluna, P,et al."The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 512.1(2022):1091-1110. |
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