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The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars

文献类型:期刊论文

作者McDonald, I33; Srinivasan, S32; Scicluna, P31; Jones, O C30; Zijlstra, A A33; Wallström, S H J29; Danilovich, T28,29,34; He JH(何金华)25,26,27; Marshall, J P24; Loon, J Th van23
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2025-07
卷号541期号:1页码:516-552
关键词catalogues surveys stars: AGB and post-AGB stars: mass-loss stars: winds, outflows
ISSN号0035-8711
DOI10.1093/mnras/staf978
产权排序第8完成单位
文献子类Article
英文摘要We provide a meta-study of the statistical and individual properties of two volume-complete sets of evolved stars in the solar neighbourhood: (1) 852 stars from the Nearby Evolved Stars Survey (NESS), and (2) a partially overlapping set of 507 evolved stars within 300 pc. We also investigate distance determinations to these stars, their luminosity functions and their spatial distribution. Gaia apsis GSP-Phot aeneas temperatures of bright giant stars often appear to be underestimated. Existing literature on asymptotic giant branch (AGB) stars undersamples both the most and least extreme nearby dust-producing stars. We reproduce the literature star formation history of the solar neighbourhood, though stellar-evolution models overpredict the number of AGB stars of ages around 500 Myr. The distribution of AGB stars broadly matches the known 300 pc scale height of the Galactic disc and shows concentration in the direction of the Galactic centre. Most dust-producing carbon stars belong to the Galactic thick-disc population.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
WOS关键词MASS-LOSS RATES ; RED GIANT BRANCH ; AGB STARS ; VARIABLE-STARS ; FUNDAMENTAL PARAMETERS ; SOLAR NEIGHBORHOOD ; INFRARED EXCESSES ; FORMATION HISTORY ; DUST PRODUCTION ; STELLAR TRACKS
资助项目Science and Technology Facilities Council; Korea Astronomy and Space Science Institute[2017YFA0402700]; National Key R&D Program of China[M17BL002]; Science and Technology Facilities Council of the United Kingdom
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001521336400001
出版者OXFORD UNIV PRESS
资助机构Science and Technology Facilities Council ; Korea Astronomy and Space Science Institute[2017YFA0402700] ; National Key R&D Program of China[M17BL002] ; Science and Technology Facilities Council of the United Kingdom
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28393]  
专题云南天文台_其他
通讯作者McDonald, I
作者单位1.SETI Institute, 189 Bernardo Avenue, Suite 100, Mountain View, CA 94043, USA;
2.National Science Foundation, 2415 Eisenhower Avenue, Alexandria, VA 22314, USA
3.NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, USA;
4.Valencian International University, Pintor Sorolla no. 21, Valencia, Valencia E-46002, Spain;
5.East Asian Observatory (JCMT), 660 N. A‘ohoku Place, Hilo, HI 96720, USA;
6.Center for General Education, Institute for Comprehensive Education, Kagoshima University, 1-21-30 Korimoto, Kagoshima 890–0065, Japan;
7.Department of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK;
8.Amanogawa Galaxy Astronomy Research Center (AGARC), Graduate School of Science and Engineering, Kagoshima University, 1-21-35 Korimoto, Kagoshima 890–0065, Japan;
9.Department of Physics and Astronomy, Kagoshima University, 1-21-35 Korimoto, Kagoshima, 890-0065, Japan;
10.AURA for the European Space Agency, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA;
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GB/T 7714
McDonald, I,Srinivasan, S,Scicluna, P,et al. The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2025,541(1):516-552.
APA McDonald, I.,Srinivasan, S.,Scicluna, P.,Jones, O C.,Zijlstra, A A.,...&Rau, G.(2025).The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,541(1),516-552.
MLA McDonald, I,et al."The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 541.1(2025):516-552.

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