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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, P.64,65; Kemper, F.63,65; McDonald, I61,62; Srinivasan, S.60,65; Trejo, A.65; Wallstrom, S. H. J.59,65; Wouterloot, J. G. A.58; Cami, J.55,56,57; Greaves, J.54; He, Jinhua51,52,53
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
通讯作者Scicluna, P.(peter.scicluna@eso.org)
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.
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 Kingdom ; Ministry of Science and Technology of Taiwan[MOST1042628-M-001-004-MY3] ; Ministry of Science and Technology of Taiwan[MOST107-2119-M-001-031-MY3] ; Ministry of Science and Technology of Taiwan[MOST109-2112-M-001-036-MY3] ; Academia Sinica[AS-IA-106-M03] ; UK Science and Technology Facilities Council[ST/L00768/1] ; UK Science and Technology Facilities Council[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)[1285221N] ; ERC[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)[ERC-2014-CoG-647939] ; STFC Ernest Rutherford fellowship[ST/L003597/1] ; Natural Sciences and Engineering Research Council (NSERC) ; National Natural Science Foundation of China[11873086] ; National Natural Science Foundation of China[U1631237] ; Yunnan Province of China[2017HC018] ; NASA[80GSFC17M0002] ; National Research Foundation of Korea (NRF) - Korea government (MIST)[2021R1A2C1008928] ; Chinese Academy of Sciences (CAS) ; [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 ; Science and Technology Facilities Council of the United Kingdom ; Ministry of Science and Technology of Taiwan ; Academia Sinica ; UK Science and Technology Facilities Council ; UK Science and Technology Facility Council ; UNAM-PAPIIT Programme ; Research Foundation Flanders (FWO) ; ERC ; EU's Horizon 2020 programme under the Marie Sklodowska-Curie grant ; Daiwa Anglo-Japan Foundation ; Great Britain Sasakawa Foundation ; European Research Council (ERC) ; STFC Ernest Rutherford fellowship ; Natural Sciences and Engineering Research Council (NSERC) ; National Natural Science Foundation of China ; Yunnan Province of China ; NASA ; National Research Foundation of Korea (NRF) - Korea government (MIST) ; Chinese Academy of Sciences (CAS)
源URL[http://ir.xao.ac.cn/handle/45760611-7/4604]  
专题星系宇宙学研究团组
通讯作者Scicluna, P.
作者单位1.Sun Yat Sen Univ, Sch Phys & Astron, 2 Daxue Rd, Zhuhai 510275, Guangdong, Peoples R China
2.SOKENDAI, Dept Space & Astronaut Sci, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan
3.JAXA, Inst Space & Astronaut Sci, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan
4.Kuffner Observ, Johann Staudstr 10, A-1160 Vienna, Austria
5.Chungbuk Natl Univ, Dept Astron & Space Sci, Cheongju 28644, South Korea
6.Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27599 USA
7.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210093, Peoples R China
8.Hainan Univ, Sch Sci, Haikou 570228, Hainan, Peoples R China
9.Catholic Univ Amer, Dept Phys, Washington, DC 20064 USA
10.NASA, Goddard Space Flight Ctr, 8800 Greenbelt Rd, 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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