日本語
 
Help Privacy Policy ポリシー/免責事項
  詳細検索ブラウズ

アイテム詳細


公開

学術論文

The radius and mass of the close solar twin 18 Scorpii derived from asteroseismology and interferometry

MPS-Authors
/persons/resource/persons16172

Asplund,  M.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

External Resource
There are no locators available
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
フルテキスト (公開)
公開されているフルテキストはありません
付随資料 (公開)
There is no public supplementary material available
引用

Bazot, M., Ireland, M. J., Huber, D., Bedding, T. R., Broomhall, A.-M., Campante, T. L., Carfantan, H., Chaplin, W. J., Elsworth, Y., Meléndez, J., Petit, P., Théado, S., Van Grootel, V., Arentoft, T., Asplund, M., Castro, M., Christensen-Dalsgaard, J., do Nascimento, J. D., Dintrans, B., Dumusque, X., Kjeldsen, H., McAlister, H. A., Metcalfe, T. S., Monteiro, M. J. P. F. G., Santos, N. C., Sousa, S., Sturmann, J., Sturmann, L., ten Brummelaar, T. A., Turner, N., & Vauclair, S. (2011). The radius and mass of the close solar twin 18 Scorpii derived from asteroseismology and interferometry. Astronomy and Astrophysics, 526:, pp. 1-4. doi:10.1051/0004-6361/201015679.


引用: https://hdl.handle.net/11858/00-001M-0000-0011-267E-C
要旨
要旨はありません