The Evolution of Massive Stars with Mass Loss: the H- and the He-burning Phases

被引：0
作者：
Chieffi, Alessandro [1 ]
Limongi, Marco [2 ]
机构：
[1] Ist Astrofis Spaziale & Fis Cosm, Ist Nazl Astrofis, I-00133 Rome, Italy
[2] Osserv Astron Roma, Ist Nazl Astrofis, I-00040 Monte Porzio Catone, Italy
来源：
JOURNAL OF THE KOREAN PHYSICAL SOCIETY | 2010年 / 56卷 / 05期
关键词：
Stars; Stellar evolution; Nucleosynthesis; WOLF-RAYET STARS; LOSS RATES; NUCLEOSYNTHESIS;
D O I：
10.3938/jkps.56.1673
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The evolution of a massive star to its final fate is strongly modified by the efficient mass loss episodes it experiences during its lifetime. In the following, we will briefly summarize how the Hand the He- burning phases depend on the adopted mass loss rate.
引用
收藏
页码：1673 / 1676
页数：4
相关论文
共 50 条
  • [41] New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars III. Updated mass-loss rates for stellar evolution
    Bjorklund, R.
    Sundqvist, J. O.
    Singh, S. M.
    Puls, J.
    Najarro, F.
    ASTRONOMY & ASTROPHYSICS, 2023, 676
  • [42] Circumstellar shells and mass loss rates: Clues to the evolution of S stars
    Jorissen, A
    Knapp, GR
    ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1998, 129 (02): : 363 - 398
  • [43] EVOLUTION OF ROTATING LOW MASS STARS WITH ANGULAR-MOMENTUM LOSS
    KIZILOGLU, N
    ASTRONOMY & ASTROPHYSICS, 1991, 243 (02) : 405 - 411
  • [44] Maximum mass-loss rates of line-driven winds of massive stars
    Aerts, C
    Lamers, HJGLM
    ASTRONOMY & ASTROPHYSICS, 2003, 403 (02) : 625 - 635
  • [45] Hydrodynamical simulations and similarity relations for eruptive mass-loss from massive stars
    Owocki, Stanley P.
    Hirai, Ryosuke
    Podsiadlowski, Philipp
    Schneider, Fabian R. N.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2019, 485 (01) : 988 - 1000
  • [46] EVOLUTION OF VERY MASSIVE POPULATION III STARS WITH MASS ACCRETION FROM PRE-MAIN SEQUENCE TO COLLAPSE
    Ohkubo, Takuya
    Nomoto, Ken'ichi
    Umeda, Hideyuki
    Yoshida, Naoki
    Tsuruta, Sachiko
    ASTROPHYSICAL JOURNAL, 2009, 706 (02) : 1184 - 1193
  • [47] Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity
    de Wit, S.
    Bonanos, A. Z.
    Antoniadis, K.
    Zapartas, E.
    Ruiz, A.
    Britavskiy, N.
    Christodoulou, E.
    De, K.
    Maravelias, G.
    Munoz-Sanchez, G.
    Tsopela, A.
    ASTRONOMY & ASTROPHYSICS, 2024, 689
  • [48] Presupernova Evolution and Explosive Nucleosynthesis of Rotating Massive Stars in the Metallicity Range-3 ≤ [Fe/H] ≤ 0
    Limongi, Marco
    Chieffi, Alessandro
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2018, 237 (01)
  • [49] Exploring the Red Supergiant wind kink A Universal mass-loss concept for massive stars
    Vink, Jorick S.
    Sabhahit, Gautham N.
    ASTRONOMY & ASTROPHYSICS, 2023, 678
  • [50] The Eddington factor as the key to understand the winds of the most massive stars Evidence for a Γ-dependence of Wolf-Rayet type mass loss
    Graefener, G.
    Vink, J. S.
    de Koter, A.
    Langer, N.
    ASTRONOMY & ASTROPHYSICS, 2011, 535
12345