Exoplanets or Dynamic Atmospheres? The Radial Velocity and Line Shape Variations of 51 Pegasi and τ Bootis-Reference-Cited by-同舟云学术

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Exoplanets or Dynamic Atmospheres? The Radial Velocity and Line Shape Variations of 51 Pegasi and τ Bootis

Published:1998-08 Issue:2 Volume:117 Page:563-585
ISSN:0067-0049
Container-title:The Astrophysical Journal Supplement Series
language:en
Short-container-title:ASTROPHYS J SUPPL S

Author:

Brown Timothy M.,Kotak Rubina,Horner Scott D.,J. Kennelly Edward,Korzennik Sylvain,Nisenson P.,Noyes Robert W.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference31 articles.

1. Abramowitz, M. & Stegun, I. 1972, Handbook of Mathematical Functions (New York: Dover)

2. Properties of Sun-like Stars with Planets: [CLC]ρ[TSUP]1[/TSUP][/CLC] Cancri, τ Bootis, and υ Andromedae

3. Mode identification from line profile variations

4. Proximity of Jupiter-Like Planets to Low-Mass Stars

5. Asteroseismology

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3. Image watermarking based on the space/spatial-frequency analysis and Hermite functions expansion;Journal of Electronic Imaging;2013-02-06

4. Pattern formation on the surface of a bubble driven by an acoustic field;Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences;2011-08-17

5. Asteroseismology;Astronomy and Astrophysics Library;2010

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