(Q59052257)

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A planetary companion for 51 Pegasi implied by absence of pulsations in the stellar spectra

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title

A planetary companion for 51 Pegasi implied by absence of pulsations in the stellar spectra (English)

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David F. Gray

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1

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English

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publication date

January 1998

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391

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6663

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153–154

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exact match

https://scigraph.springernature.com/pub.10.1038/34365

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cites work

A Jupiter-mass companion to a solar-type star

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Crossref

reference URL

https://api.crossref.org/works/10.1038%2F34365

retrieved

21 January 2018

The Planet around 51 Pegasi

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Crossref

reference URL

https://api.crossref.org/works/10.1038%2F34365

retrieved

21 January 2018

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

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reference URL

https://api.crossref.org/works/10.1038%2F34365

retrieved

21 January 2018

Further evidence for the planet around 51 Pegasi

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Crossref

reference URL

https://api.crossref.org/works/10.1038%2F34365

retrieved

21 January 2018

Nonradial oscillation in the solar-temperature star 51 Pegasi

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reference URL

https://api.crossref.org/works/10.1038%2F34365

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7 January 2021

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A new approach to periodogram analyses

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reference URL

https://api.crossref.org/works/10.1038%2F34365

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7 January 2021

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inferred from DOI database lookup

Spectral line-depth ratios as temperature indicators for cool stars

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https://api.crossref.org/works/10.1038%2F34365

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7 January 2021

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1016433530

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(Q59052257)

A planetary companion for 51 Pegasi implied by absence of pulsations in the stellar spectra

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