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Volumn 349, Issue 1, 1999, Pages 220-224

Line profile variation and planets around 51 Pegasi and ν Andromedae

Author keywords

Planets and satellites: general; Stars: individual: And; Stars: individual: 51 Peg; Techniques: radial velocities; Techniques: spectroscopic

Indexed keywords


EID: 4143059223     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (3)

References (27)
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    • Gonzalez G., 1998, A&A 334, 221
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  • 13
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    • (1998) Nat , vol.391 , pp. 153
    • Gray, D.F.1
  • 21
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    • Central Bureau for Astr. Telegrams, Smithsonian Astrophys. Obs., Cambridge, USA
    • Mayor M., Queloz D., Marcy G., et al., 1995, IAU Circ. 6251, Central Bureau for Astr. Telegrams, Smithsonian Astrophys. Obs., Cambridge, USA
    • (1995) IAU Circ. , vol.6251
    • Mayor, M.1    Queloz, D.2    Marcy, G.3
  • 22
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    • A Search for Substellar companion to Solartype Stars via Precise Doppler Measurements: A first Jupiter Mass Companion Detected. 1996
    • Pallavicini R., Dupree A.K. (eds.) Cool Stars, Stellar Systems, and the Sun. 9th Cambridge Workshop
    • Mayor M., Queloz D., A Search for Substellar companion to Solartype Stars via Precise Doppler Measurements: A first Jupiter Mass Companion Detected. 1996, In: Pallavicini R., Dupree A.K. (eds.) Cool Stars, Stellar Systems, and the Sun. 9th Cambridge Workshop, ASP Conference Series vol. 109, p. 35
    • ASP Conference Series , vol.109 , pp. 35
    • Mayor, M.1    Queloz, D.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.