A planetary companion for 51 Pegasi implied by absence of pulsations in the stellar spectra
- 1 January 1998
- journal article
- letter
- Published by Springer Nature in Nature
- Vol. 391 (6663) , 153-154
- https://doi.org/10.1038/34365
Abstract
No abstract availableKeywords
This publication has 7 references indexed in Scilit:
- Further evidence for the planet around 51 PegasiNature, 1998
- Non‐Radial Oscillation in the Solar‐Temperature Star 51 PegasiThe Astrophysical Journal, 1997
- The Planet around 51 PegasiThe Astrophysical Journal, 1997
- Absence of a planetary signature in the spectra of the star 51 PegasiNature, 1997
- A Jupiter-mass companion to a solar-type starNature, 1995
- Spectral line-depth ratios as temperature indicators for cool starsPublications of the Astronomical Society of the Pacific, 1994
- A new approach to periodogram analyses.The Astrophysical Journal, 1973