Synapse
⌘+K
Synapse
PulseExploreClubsResearchersJournals
Instagram
HomeClubsExplore
January 20, 2000The Astrophysical Journal

A Transiting “51 Peg–like” Planet

View Full Paper
Ask AI
Bookmark
Share

Authors

GHGregory W. HenryTenneco (United States)GMGeoffrey W. MarcyBrigham Young UniversityRBR. Paul ButlerRutherford Appleton Laboratory

Discussion

Loading...

Member takes

Implication

Key Points

Key points are not available for this paper at this time.

Cite This Study

Henry et al. (2000) studied this question.

synapsesocial.com/papers/6a63bcdba98bc91ae4c1b4f2https://doi.org/10.1086/312458
View Full Paper
Ask AI
Bookmark
Share

Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

  1. 1Rotation, convection, and magnetic activity in lower main-sequence stars1984 · 1,727 citations
  2. 2A Planet with a 3.1 Day Period around a Solar Twin1998 · 105 citations
  3. 3Properties of Sun‐like Stars with Planets: 51 Pegasi, 47 Ursae Majoris, 70 Virginis, and HD 1147621997 · 68 citations
  4. 4Magnetic Activity–related Radial Velocity Variations in Cool Stars: First Results from the Lick Extrasolar Planet Survey1998 · 316 citations
  5. 5Precision radial velocities with an iodine absorption cell1992 · 436 citations