The evolution of the internal rotation of solar-type stars

被引：0
作者：
Di Mauro, Maria Pia [1 ]
Ventura, Rita [2 ]
Cardini, Daniela [1 ]
Christensen-Dalsgaard, Jorgen [3 ]
Dziembowski, Wojciech A. [4 ]
Paterno, Lucio
机构：
[1] INAF, IAPS Ist Astrofis & Planetol Spaziali, Via Fosso Cavaliere 100, I-00133 Rome, Italy
[2] INAF, Astrophys Observ Catania, I-95020 Catania, Italy
[3] Aarhus Univ, Dept Phys & Astron, Stellar Astrophys Ctr, DK-8000 Aarhus C, Denmark
[4] Univ Warsaw Observ, PL-00478 Warsaw, Poland
来源：
PRECISION ASTEROSEISMOLOGY | 2014年 / 9卷 / 301期
关键词：
stars: oscillations; stars: rotation; stars: evolution; Sun: helioseismology; Sun: evolution; Sun: rotation;
D O I：
10.1017/S1743921313014567
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We discuss the potential of asteroseismic inversion to study the internal dynamics of solar-type stars and to reconstruct the evolution of the internal rotation from the main sequence to the red-giant phase. In particular, we consider the use of gravity and mixed modes and the application of different inversion methods.
引用
收藏
页码：345 / 348
页数：4
相关论文
共 50 条
  • [21] Asteroseismic modelling of solar-type stars: Internal systematics from input physics and surface correction methods
    Nsamba B.
    Campante T.L.
    Monteiro M.J.P.F.G.
    Cunha M.S.
    Rendle B.M.
    Reese D.R.
    Verma K.
    Nsamba, B. (benard.nsamba@astro.up.pt), 2018, Oxford University Press (477) : 5052 - 5063
  • [22] Asteroseismology of solar-type stars: signatures of convective and/or helium cores
    Soriano, M.
    Vauclair, S.
    ASTRONOMY & ASTROPHYSICS, 2008, 488 (03) : 975 - 985
  • [23] Effects of rotational mixing on the asteroseismic properties of solar-type stars
    Eggenberger, P.
    Meynet, G.
    Maeder, A.
    Miglio, A.
    Montalban, J.
    Carrier, F.
    Mathis, S.
    Charbonnel, C.
    Talon, S.
    ASTRONOMY & ASTROPHYSICS, 2010, 519
  • [24] Tidal dissipation in rotating solar-type stars
    Ogilvie, G. I.
    Lin, D. N. C.
    ASTROPHYSICAL JOURNAL, 2007, 661 (02) : 1180 - 1191
  • [25] ON A STOCHASTIC MODEL FOR THE SPIN-DOWN OF SOLAR-TYPE STARS
    Leprovost, Nicolas
    Kim, Eun-jin
    ASTROPHYSICAL JOURNAL, 2010, 719 (01) : 287 - 298
  • [26] Lithium depletion and angular momentum transport in solar-type stars
    Dumont, T.
    Palacios, A.
    Charbonnel, C.
    Richard, O.
    Amard, L.
    Augustson, K.
    Mathis, S.
    ASTRONOMY & ASTROPHYSICS, 2021, 646
  • [27] DYNAMICAL MODEL FOR SPINDOWN OF SOLAR-TYPE STARS
    Sood, Aditi
    Kim, Eun-jin
    Hollerbach, Rainer
    ASTROPHYSICAL JOURNAL, 2016, 832 (02)
  • [28] Activity trends in young solar-type stars
    Lehtinen, J.
    Jetsu, L.
    Hackman, T.
    Kajatkari, P.
    Henry, G. W.
    ASTRONOMY & ASTROPHYSICS, 2016, 588
  • [29] Spectrum and amplitudes of internal gravity waves excited by penetrative convection in solar-type stars
    Dintrans, B
    Brandenburg, A
    Nordlund, Å
    Stein, RF
    ASTRONOMY & ASTROPHYSICS, 2005, 438 (01) : 365 - 376
  • [30] Transition of latitudinal differential rotation as a possible cause of weakened magnetic braking of solar-type stars
    Tokuno, Takato
    Suzuki, Takeru K.
    Shoda, Munehito
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023, 520 (01) : 418 - 436
12345