Could very low-metallicity stars with rotation-dominated orbits have been driven by the bar?

被引：0

作者：

Yuan, Zhen ^{[1
]}

Li, Chengdong ^{[1
]}

Martin, Nicolas F. ^{[1
,2
]}

Monari, Giacomo ^{[1
]}

Famaey, Benoit ^{[1
]}

Siebert, Arnaud ^{[1
]}

Chiba, Rimpei ^{[3
]}

Ardern-Arentsen, Anke ^{[4
]}

Sestito, Federico ^{[5
]}

Thomas, Guillaume F. ^{[6
,7
]}

Hill, Vanessa ^{[8
]}

Ibata, Rodrigo A. ^{[1
]}

Kordopatis, Georges ^{[8
]}

Starkenburg, Else ^{[9
]}

Viswanathan, Akshara ^{[9
]}

机构：

[1] Université de Strasbourg, CNRS, Observatoire Astronomique de Strasbourg, UMR 7550, Strasbourg,F-67000, France

[2] Max-Planck-Institut für Astronomie, Königstuhl 17, Heidelberg,D-69117, Germany

[3] Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St George Street, Toronto,ON,M5S 3H8, Canada

[4] Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge,CB3 0HA, United Kingdom

[5] Dept. of Physics and Astronomy, University of Victoria, P.O. Box 3055, STN CSC, Victoria,BC,V8W 3P6, Canada

[6] Instituto de Astrofísica de Canarias, Tenerife, La Laguna,E-38205, Spain

[7] Universidad de la Laguna, Dept. Astrofísica, Tenerife, La Laguna,E-38206, Spain

[8] Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Nice, France

[9] Kapteyn Astronomical Institute, University of Groningen, Landleven 12, Groningen,9747 AD, Netherlands

来源：

Astronomy and Astrophysics | 2024年 / 691卷

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引用

共 14 条

[1] Could very low-metallicity stars with rotation-dominated orbits have been driven by the bar?
Yuan, Zhen
Li, Chengdong
Martin, Nicolas F.
Monari, Giacomo
Famaey, Benoit
Siebert, Arnaud
Chiba, Rimpei
Ardern-Arentsen, Anke
Sestito, Federico
Thomas, Guillaume F.
Hill, Vanessa
Ibata, Rodrigo A.
Kordopatis, Georges
Starkenburg, Else
Viswanathan, Akshara
ASTRONOMY & ASTROPHYSICS, 2024, 691
[2] Effects of rotation in low-metallicity stars
Heap, SR
Lanz, T
STELLAR ROTATION, 2004, (215): : 220 - 221
[3] Mass loss and very low-metallicity stars
Hirschi, Raphael
Chiappini, Cristina
Meynet, Georges
Ekstrom, Sylvia
Maeder, Andre
UNSOLVED PROBLEMS IN STELLAR PHYSICS: A CONFERENCE IN HONOUR OF DOUGLAS GOUGH, 2007, 948 : 397 - 404
[4] Low-metallicity massive single stars with rotation Evolutionary models applicable to I Zwicky 18
Szecsi, Dorottya
Langer, Norbert
Yoon, Sung-Chul
Sanyal, Debashis
de Mink, Selma
Evans, Christopher J.
Dermine, Tyl
ASTRONOMY & ASTROPHYSICS, 2015, 581
[5] Low-metallicity massive single stars with rotation: Evolutionary models applicable to i Zwicky 18
Szécsi, Dorottya
Langer, Norbert
Yoon, Sung-Chul
Sanyal, Debashis
De Mink, Selma
Evans, Christopher J.
Dermine, Tyl
Astronomy and Astrophysics, 2015, 581
[6] Evolution of massive stars at very low metallicity, including rotation and binary interactions
Yoon, S. -C
Cantiello, M.
Langer, N.
FIRST STARS III, 2008, 990 : 225 - +
[7] Star clusters forming in a low-metallicity starburst - rapid self-enrichment by (very) massive stars
Lahen, Natalia
Naab, Thorsten
Szecsi, Dorottya
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2024, 530 (01) : 645 - 667
[8] Very low-metallicity massive stars: Pre-SN evolution models and primary nitrogen production
Hirschi, R.
Astronomy and Astrophysics, 1600, 461 (02): : 571 - 583
[9] Discovery of an ''alpha'' element-poor halo star in a search for very low-metallicity disk stars
Carney, BW
Wright, JS
Sneden, C
Laird, JB
Aguilar, LA
Latham, DW
ASTRONOMICAL JOURNAL, 1997, 114 (01): : 363 - 375
[10] Very low-metallicity massive stars: Pre-SN evolution models and primary nitrogen production
Hirschi, R.
ASTRONOMY & ASTROPHYSICS, 2007, 461 (02): : 571 - U21

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