Absence of a planetary signature in the spectra of the star 51 Pegasi-Reference-Cited by-同舟云学术

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Absence of a planetary signature in the spectra of the star 51 Pegasi

Published:1997-02 Issue:6619 Volume:385 Page:795-796
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Gray David F.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/385795a0.pdf

Reference27 articles.

1. Mayor, M. & Queloz, D. A Jupiter-mass companion to a solar-type star. Nature 378, 355–359 (1995).

2. Marcy, G. W. et al. The planet around 51 Pegasi. Astrophys. J. (submitted).

3. Gray, D. F., Baliunas, S. L., Lockwood, G. W. & Skiff, B. A. Variations of β Comae through a magnetic minimum. Astrophys. J. 456, 365–369 (1996).

4. Gray, D. F., Baliunas, S. L., Lockwood, G. W. & Skiff, B. A. Magnetic, photometric, temperature, and granulation variations of ξ Boo A 1984–1993. Astrophys. J. 465, 945–950 (1996).

5. Gray, D. F. in Instrumentation and Research Programmes for Small Telescopes (eds Hearnshaw, J. B. & Cottrell, P. L.) 401–412 (Reidel, Dordrecht, 1986).

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