WISE J104915.57-531906.1
出典: フリー百科事典『ウィキペディア（Wikipedia）』 (2019/07/07 05:05 UTC 版)
WISE J104915.57-531906.1とは、地球から見てほ座の方向に約6.52光年離れた位置にある褐色矮星同士の二重星である。名称が長いので通常WISE 1049-5319と略される[1][2]。
- ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag Discovery of a Binary Brown Dwarf at 2 parsecs from the Sun Penn State Science
- ^ a b c d The Closest Star System Found in a Century Penn State Science
- ^ a b c Howdy, Neighbor! New Twin Stars Are Third Closest to the Sun Slate
- ^ a b c d e f g h Individual, Model-Independent Masses of the Closest Known Brown Dwarf Binary to the Sun arXiv
- ^ On the Nearby Binary Brown Dwarf WISE J104915.57-531906.1 (Luhman 16) arXiv
- ^ Marsh, Kenneth A.; Wright, Edward L.; Kirkpatrick, J. Davy; Gelino, Christopher R.; Cushing, Michael C.; Griffith, Roger L.; Skrutskie, Michael F.; Eisenhardt, Peter R. (2013). “PARALLAXES AND PROPER MOTIONS OF ULTRACOOL BROWN DWARFS OF SPECTRAL TYPES Y AND LATE T”. The Astrophysical Journal 762 (2): 119. arXiv:1211.6977. doi:10.1088/0004-637X/762/2/119. ISSN 0004-637X.
- ^ Luhman, Kevin L. (2014-04-21). “Discovery of a ~250 K Brown Dwarf at 2 pc from the Sun”. Astrophysical Journal Letters 786 (2): L18. arXiv:1404.6501. Bibcode: 2014ApJ...786L..18L. doi:10.1088/2041-8205/786/2/L18.
- ^ Luhman, Kevin L.; Esplin, Taran L. (2016-09). “The Spectral Energy Distribution of the Coldest Known Brown Dwarf”. Astronomical Journal 152 (2): 78. arXiv:1605.06655. Bibcode: 2016AJ....152...78L. doi:10.3847/0004-6256/152/3/78.
- ^ WISE Nabs the Closest Brown Dwarfs Yet Discovered Universe Today
[続きの解説]
「WISE J104915.57-531906.1」の続きの解説一覧
- 1 WISE J104915.57-531906.1とは
- 2 WISE J104915.57-531906.1の概要
- 3 距離
- 4 発見
- 5 出典
- WISE J104915.57-531906.1のページへのリンク
