A Planet with a 3.1 Day Period around a Solar Twin-Reference-Cited by-同舟云学术

A Planet with a 3.1 Day Period around a Solar Twin

Published:1998-12 Issue:754 Volume:110 Page:1389-1393
ISSN:0004-6280
Container-title:Publications of the Astronomical Society of the Pacific
language:en
Short-container-title:PUBL ASTRON SOC PAC

Author:

Butler R. Paul,Marcy Geoffrey W.,Vogt Steven S.,Apps Kevin

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/1538-3873/110/i=754/a=1389/pdf

Reference33 articles.

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

2. A Search for Line Shape and Depth Variations in 51 Pegasi and τ Bootis

3. Burrows, A., etal 1997, in ASP Conf. Ser. 134, Brown Dwarfs and Extrasolar Planets, ed. R. Rebolo, E. Martin, & M. R. Zapatero Osorio (San Francisco: ASP), 354

4. Three New “51 Pegasi–Type” Planets

5. Attaining Doppler Precision of 3 M s-1

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