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The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope
Scicluna, P1,2; Kemper, F1,3; McDonald, I4,5; Srinivasan, S1,6; Trejo, A1; Wallström, S H J1,7; Wouterloot, J G A8; Cami, J9,10,11; Greaves, J12; He JH(何金华)13,14,15; Hoai, D T16,17; Kim, Hyosun18; Jones, O C19; Shinnaga, H20,21; Clark, C J R22; Dharmawardena, T1,23; Holland, W19; Imai, H21,24; Loon, J Th van25; Menten, K M26; Wesson, R27; Chawner, H12; Feng, S28; Goldman, S22; Liu, F C29; MacIsaac, H9,10; Tang, J28,30; Zeegers, S1; Amada, K20; Antoniou, V31,32; Bemis, A33; Boyer, M L22; Chapman, S34; Chen, X35; Cho, S-H18; Cui, L36; Dell’Agli, F37; Friberg, P8; Fukaya, S20; Gomez, H12; Gong, Y26; Hadjara, M14,15; Haswell, C5; Hirano, N1; Hony, S38; Izumiura, H39; Jeste, M26; Jiang, X40; Kaminski, T32; Keaveney, N41; Kim, J18,35; Kraemer, K E42; Kuan, Y-J1,29; Lagadec, E43; Lee, C F1; Li, D44,45,46; Liu, S-Y1; Liu, T35; Looze, I de27,47; Lykou, F48,49; Maraston, C50; Marshall, J P1,51; Matsuura, M12; Min, C52; Otsuka, M1,53; Oyadomari, M20; Parsons, H8; Patel, N A32; Peeters, E9,10,11; Pham, T A16; Qiu, J33,54; Randall, S3; Rau, G55,56; Redman, M P41; Richards, A M S4; Serjeant, S5; Shi, C57,58; Sloan, G C22,59; Smith, M W L12; Suh, K-W60; Toalá, J A6; Uttenthaler, S61; Ventura, P36; Wang, B44; Yamamura, I62,63; Yang, T36; Yun, Y18; Zhang FH(张奉辉)13; Zhang, Y49,64; Zhao, G44; Zhu, M44; Zijlstra, A A4
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2022-04-04
卷号512期号:1页码:1091-1110
DOI10.1093/mnras/stab2860
产权排序第13完成单位
收录类别SCI ; EI
关键词catalogues surveys stars: AGB and post-AGB stars: mass-loss stars: winds outflows
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.

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]
项目资助者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]
语种英语
学科领域天文学 ; 恒星与银河系 ; 恒星形成与演化
文章类型Article
出版者OXFORD UNIV PRESS
出版地GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
ISSN0035-8711
URL查看原文
WOS记录号WOS:000778666900001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]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
EI入藏号20221712041272
EI主题词Surveys
EI分类号451.1 Air Pollution Sources - 657.2 Extraterrestrial Physics and Stellar Phenomena - 711 Electromagnetic Waves
引用统计
被引频次：8[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/25037
专题其他
大样本恒星演化研究组
通讯作者Scicluna, P
作者单位1.Institute of Astronomy and Astrophysics, Academia Sinica, 11F of AS/NTU Astronomy-Mathematics Building, No. 1, Section 4, Roosevelt Rd, Taipei 10617, Taiwan;
2.European Southern Observatory, Alonso de Cordova 3107, Santiago RM, Chile;
3.European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching b. München, Germany;
4.Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, School of Natural Sciences, University of Manchester, M13 9PL Manchester, UK;
5.Department of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK;
6.Instituto de Radioastronomía y Astrofísica, UNAM. Apdo. Postal 72-3 (Xangari), Morelia, Michoacán 58089, Michoacán, Mexico;
7.Institute of Astronomy, KU Leuven, Celestijnenlaan 200D bus 2401, B-3001 Leuven, Belgium;
8.East Asian Observatory (JCMT), 660 N. A‘ohoku Place, Hilo, HI 96720, USA;
9.Department of Physics and Astronomy, University of Western Ontario, London, ON N6A 3K7, Canada;
10.Institute for Earth and Space Exploration, University of Western Ontario, London, ON N6A 3K7, Canada;
11.SETI Institute, 189 Bernardo Avenue, Suite 100, Mountain View, CA 94043, USA;
12.School of Physics and Astronomy, Cardiff University, The Parade, Cardiff CF24 3AA, UK;
13.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, China;
14.Chinese Academy of Sciences South America Center for Astronomy, National Astronomical Observatories, CAS, Beijing 100101, China;
15.Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile;
16.Department of Astrophysics, Vietnam National Space Center (VNSC), Vietnam Academy of Science and Technology (VAST), 18 Hoang Quoc Viet, Cau Giay, Ha Noi, Viet Nam;
17.Graduate University of Science and Technology (GUST), Vietnam Academy of Science and Technology (VAST), 18 Hoang Quoc Viet, Cau Giay, Ha Noi, Viet Nam;
18.Korea Astronomy and Space Science Institute (KASI) 776, Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of Korea;
19.UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK;
20.Department of Physics and Astronomy, Kagoshima University, 1-21-35 Korimoto, Kagoshima, Japan;
21.Amanogawa Galaxy Astronomy Research Center (AGARC), Graduate School of Science and Engineering, Kagoshima University, 1-21-35 Korimoto, Kagoshima 890-0065, Japan;
22.Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA;
23.Max-Planck-Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg, Germany;
24.Center for General Education, Institute for Comprehensive Education, Kagoshima University, 1-21-30 Korimoto, Kagoshima 890-0065, Japan;
25.Lennard-Jones Laboratories, Keele University, Keele ST5 5BG, UK;
26.Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany;
27.Department of Physics and Astronomy, University College London, Gower St, London WC1E 6BT, UK;
28.National Astronomical Observatory of China, Datun Road 20, Chaoyang, Beijing 100012, China;
29.Department of Earth Sciences, National Taiwan Normal University, Taipei 11677, Taiwan;
30.CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Science, Beijing 100101, China;
31.Department of Physics and Astronomy, Texas Tech University, Box 41051, Lubbock, TX 79409-1051, USA;
32.Center for Astrophysics | Harvard and Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA;
33.Department of Physics and Astronomy, McMaster University, Hamilton, ON L8S 4M1, Canada;
34.Department of Physics and Atmospheric Science, Dalhousie University, Halifax, NS B3H 4R2, Canada;
35.Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China;
36.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150 Science 1-Street, 830011 Urumqi, China;
37.INAF, Osservatorio Astronomico di Roma, Via Frascati 33, I-00077 Monte Porzio Catone (RM), Italy;
38.Institut für Theoretische Astrophysik, Zentrum für Astronomie der Universität Heidelberg, Albert-Überle-Strasse 2, D-69120 Heidelberg, Germany;
39.Okayama Branch Office, Subaru Telescope, NAOJ, NINS 3037-5 Honjo, Kamogata, Asakuchi, Okayama 719-0232, Japan;
40.Department of Astronomy and Institute of Theoretical Physics and Astrophysics, Xiamen University, Fujian 361005, China;
41.Centre for Astronomy, School of Physics, National University of Ireland Galway, Galway H91 CF50, Ireland;
42.Institute for Scientific Research, Boston College, 140 Commonwealth Avenue, Chestnut Hill, MA 02467, USA;
43.Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Lagrange, 96 Bd de l'Observatoire, 06300 Nice, France;
44.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;
45.Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;
46.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 101408, China;
47.Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281 S9, B-9000 Gent, Belgium;
48.Department of Physics, The University of Hong Kong, Pok Fu Lam Road, Hong Kong SAR, China;
49.Laboratory for Space Research, The University of Hong Kong, Pok Fu Lam Road, Hong Kong SAR, China;
50.Institute of Cosmology and Gravitation, University of Portsmouth, Burnaby Road, PO1 3FX Portsmouth, UK;
51.Centre for Astrophysics, University of Southern Queensland, West Street, Toowoomba, QLD 4350, Australia;
52.Department of Astronomical Sciences, The Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan;
53.Okayama Observatory, Kyoto University, Kamogata, Asakuchi, Okayama 719-0232, Japan;
54.School of Astronomy and Space Science, Nanjing University, Nanjing 210093, China;
55.NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, USA;
56.Department of Physics, The Catholic University of America, Washington, DC 20064, USA;
57.School of Sciences, Hainan University, Hainan 570228, China;
58.Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Ministry of Education, Nanjing 210093, China;
59.Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599-3255, USA;
60.Department of Astronomy and Space Science, CHUNGBUK NATIONAL UNIVERSITY, Cheongju-City, 28644, Republic of Korea;
61.Kuffner Observatory, Johann-Staudstrasse 10, A-1160 Vienna, Austria;
62.Institute of Space and Astronautical Science, JAXA, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan;
63.Department of Space and Astronautical Science, SOKENDAI, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan;
64.School of Physics and Astronomy, Sun Yat-sen University, 2 Daxue Road, Tangjia, Zhuhai, Guangdong 510275, China
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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