Determination of three-dimensional spin–orbit angle with joint analysis of asteroseismology, transit lightcurve, and the Rossiter–McLaughlin effect: Cases of HAT-P-7 and Kepler-25-Reference-Cited by-同舟云学术

Determination of three-dimensional spin–orbit angle with joint analysis of asteroseismology, transit lightcurve, and the Rossiter–McLaughlin effect: Cases of HAT-P-7 and Kepler-25

Published:2014-10-01 Issue:5 Volume:66 Page:
ISSN:2053-051X
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Benomar Othman,Masuda Kento,Shibahashi Hiromoto,Suto Yasushi

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/66/5/94/7987381/psu069.pdf

Reference93 articles.

1. Asteroseismology

2. OBLIQUITIES OF HOT JUPITER HOST STARS: EVIDENCE FOR TIDAL INTERACTIONS AND PRIMORDIAL MISALIGNMENTS

3. LOW STELLAR OBLIQUITIES IN COMPACT MULTIPLANET SYSTEMS

4. CoRoT sounds the stars: p-mode parameters of Sun-like oscillations on HD 49933

5. Oscillation mode frequencies of 61 main-sequence and subgiant stars observed byKepler

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