文献
J-GLOBAL ID:202002225547681304
整理番号:20A0336108
近傍の若い星TW Piscis Austrini(Fomalhaut B)に対する惑星質量の可能性のある天文学的特徴:天文学,放射速度,直接イメージングからの制約【JST・京大機械翻訳】
The Possible Astrometric Signature of a Planetary-mass Companion to the Nearby Young Star TW Piscis Austrini (Fomalhaut B): Constraints from Astrometry, Radial Velocities, and Direct Imaging
著者 (9件):
De Rosa Robert J.
(Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305, USA)
,
Esposito Thomas M.
(Department of Astronomy, University of California, Berkeley, CA 94720, USA)
,
Hirsch Lea A.
(Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305, USA)
,
Nielsen Eric L.
(Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305, USA)
,
Marley Mark S.
(NASA Ames Research Center, MS 245-3, Mountain View, CA 94035, USA)
,
Kalas Paul
(Department of Astronomy, University of California, Berkeley, CA 94720, USA)
,
Kalas Paul
(SETI Institute, Carl Sagan Center, 189 Bernardo Avenue, Mountain View, CA 94043, USA)
,
Wang Jason J.
(Department of Astronomy, California Institute of Technology, Pasadena, CA 91125, USA)
,
Macintosh Bruce
(Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305, USA)
資料名:
Astronomical Journal
(Astronomical Journal)
巻:
158
号:
6
ページ:
225 (13pp)
発行年:
2019年
JST資料番号:
W1567A
ISSN:
1538-3881
資料種別:
逐次刊行物 (A)
記事区分:
原著論文
発行国:
イギリス (GBR)
言語:
英語 (EN)