Non-LTE abundance corrections for late-type stars from 2000 A to 3 μm: I. Na, Mg, and Al

被引：0
|
作者：
Lind, K. [1 ]
Nordlander, T. [2 ,3 ]
Wehrhahn, A. [4 ]
Montelius, M. [5 ]
Osorio, Y. [6 ,7 ,8 ]
Barklem, P.S. [4 ]
Afşar, M. [9 ,10 ]
Sneden, C. [10 ]
Kobayashi, C. [11 ]
机构：
[1] Department of Astronomy, Stockholm University, AlbaNova University Center, Stockholm,106 91, Sweden
[2] Centre of Excellence for Astrophysics in Three Dimensions (ASTRO-3D), Australia
[3] Research School of Astronomy and Astrophysics, Australian National University, Canberra,ACT,2611, Australia
[4] Department of Physics and Astronomy, Uppsala University, Box 516, Uppsala,75120, Sweden
[5] Kapteyn Astronomical Institute, University of Groningen, Landleven 12, Groningen,9747 AD, Netherlands
[6] Isaac Newton Group, Apartado 321, Santa Cruz de La Palma,38700, Spain
[7] Instituto de Astrofísicade Canarias, Tenerife, La Laguna,38205, Spain
[8] Departamento de Astrofísica, Universidad de la Laguna, Tenerife, La Laguna,38206, Spain
[9] Department of Astronomy and Space Sciences, Ege University, Izmir, Bornova,35100, Turkey
[10] Department of Astronomy and McDonald Observatory, The University of Texas, Austin,TX,78712, United States
[11] Centre for Astrophysics Research, Department of Physics, Astronomy and Mathematics, University of Hertfordshire, Hatfield,AL10 9AB, United Kingdom
来源：
Astronomy and Astrophysics | 2022年 / 665卷
关键词：
Stars;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
引用
收藏
相关论文
共 42 条
  • [1] Non-LTE abundance corrections for late-type stars from 2000 Å to 3 μm
    Lind, K.
    Nordlander, T.
    Wehrhahn, A.
    Montelius, M.
    Osorio, Y.
    Barklem, P. S.
    Afsar, M.
    Sneden, C.
    Kobayashi, C.
    ASTRONOMY & ASTROPHYSICS, 2022, 665
  • [2] A non-LTE analysis of Mg I lines in the atmospheres of late-type stars
    Mashonkina, LI
    Shimanskaya, NN
    Sakhibullin, NA
    ASTRONOMICHESKII ZHURNAL, 1996, 73 (02): : 212 - 220
  • [3] Non-LTE analysis of K I in late-type stars
    Reggiani, Henrique
    Amarsi, Anish M.
    Lind, Karin
    Barklem, Paul S.
    Zatsarinny, Oleg
    Bartschat, Klaus
    Fursa, Dmitry, V
    Bray, Igor
    Spina, Lorenzo
    Melendez, Jorge
    ASTRONOMY & ASTROPHYSICS, 2019, 627
  • [4] Non-LTE aluminium abundances in late-type stars
    Nordlander, T.
    Lind, K.
    ASTRONOMY & ASTROPHYSICS, 2017, 607
  • [5] Non-LTE calculations for neutral Na in late-type stars using improved atomic data
    Lind, K.
    Asplund, M.
    Barklem, P. S.
    Belyaev, A. K.
    ASTRONOMY & ASTROPHYSICS, 2011, 528
  • [6] CI non-LTE spectral line formation in late-type stars
    Fabbian, D.
    Asplund, M.
    Carlsson, M.
    CHEMICAL ABUNDANCES AND MIXING IN STARS IN THE MILKY WAY AND ITS SATELLITES, 2006, : 52 - +
  • [7] The non-LTE line formation of neutral carbon in late-type stars
    Fabbian, D.
    Asplund, M.
    Carlsson, M.
    Kiselman, D.
    ASTRONOMY & ASTROPHYSICS, 2006, 458 (03) : 899 - 914
  • [8] Spectral diagnostics of late-type stars: Non-LTE and ⟨3D⟩ approach
    Bergemann, M.
    Lind, K.
    Collet, R.
    Asplund, M.
    Magic, Z.
    ASSEMBLING THE PUZZLE OF THE MILKY WAY, 2012, 19
  • [9] Non-LTE abundance corrections of iron and carbon in A-type and related stars
    RentzschHolm, I
    ASTRONOMY & ASTROPHYSICS, 1996, 312 (03) : 966 - 972
  • [10] Non-LTE line formation of Fe in late-type stars - I. Standard stars with 1D and ⟨3D⟩ model atmospheres
    Bergemann, Maria
    Lind, K.
    Collet, R.
    Magic, Z.
    Asplund, M.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 427 (01) : 27 - 49
12345