Photometric and CaiiH and K Spectroscopic Variations in Nearby Sun‐like Stars with Planets. III.
- 1 March 2000
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 531 (1), 415-437
- https://doi.org/10.1086/308466
Abstract
No abstract availableKeywords
This publication has 65 references indexed in Scilit:
- Evidence for Multiple Companions to υ AndromedaeThe Astrophysical Journal, 1999
- Evolution of the Solar Nebula. IV. Giant Gaseous Protoplanet FormationThe Astrophysical Journal, 1998
- A Search for Line Shape and Depth Variations in 51 Pegasi and τ BootisThe Astrophysical Journal, 1998
- Giant Planet Formation by Gravitational InstabilityScience, 1997
- Properties of Sun-like Stars with Planets: [CLC]ρ[TSUP]1[/TSUP][/CLC] Cancri, τ Bootis, and υ AndromedaeThe Astrophysical Journal, 1997
- A Planet Orbiting 47 Ursae MajorisThe Astrophysical Journal, 1996
- Chromospheric variations in main-sequence starsThe Astrophysical Journal, 1995
- Effective temperatures of M dwarfsThe Astrophysical Journal, 1992
- Evidence for long-term brightness changes of solar-type starsNature, 1990
- Time-series measurements of chromospheric CA II H and K emission in cool stars and the search for differential rotationThe Astrophysical Journal, 1985