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The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope

文献类型：期刊论文

作者Scicluna, P63,64; Kemper, F62,64; McDonald, I60,61; Srinivasan, S59,64; Trejo, A64; Wallström, S H J58,64; Wouterloot, J G A57; Cami, J54,55,56; Greaves, J53; He JH(何金华)50,51,52
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2022-04-04
卷号512期号:1页码:1091-1110
ISSN号0035-8711
关键词catalogues surveys stars: AGB and post-AGB stars: mass-loss stars: winds outflows
DOI10.1093/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
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
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]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/25037]  
专题云南天文台_其他
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.School of Physics and Astronomy, Sun Yat-sen University, 2 Daxue Road, Tangjia, Zhuhai, Guangdong 510275, China
2.Department of Space and Astronautical Science, SOKENDAI, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan;
3.Institute of Space and Astronautical Science, JAXA, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan;
4.Kuffner Observatory, Johann-Staudstrasse 10, A-1160 Vienna, Austria;
5.Department of Astronomy and Space Science, CHUNGBUK NATIONAL UNIVERSITY, Cheongju-City, 28644, Republic of Korea;
6.Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599-3255, USA;
7.Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Ministry of Education, Nanjing 210093, China;
8.School of Sciences, Hainan University, Hainan 570228, China;
9.Department of Physics, The Catholic University of America, Washington, DC 20064, USA;
10.NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, USA;
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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