Probable detection of starlight reflected from the giant planet orbiting τ Boötis
- 1 December 1999
- journal article
- research article
- Published by Springer Science and Business Media LLC in Nature
- Vol. 402 (6763), 751-755
- https://doi.org/10.1038/45451
Abstract
No abstract availableOther Versions
This publication has 12 references indexed in Scilit:
- An Upper Limit on the Reflected Light from the Planet Orbiting the Star τ BootisThe Astrophysical Journal, 1999
- Planetary Companions around Two Solar‐Type Stars: HD 195019 and HD 217107Publications of the Astronomical Society of the Pacific, 1999
- A Planet with a 3.1 Day Period around a Solar TwinPublications of the Astronomical Society of the Pacific, 1998
- Spectral Line Distortions in the Presence of a Close-in PlanetThe Astrophysical Journal, 1998
- Spectropolarimetric observations of active starsMonthly Notices of the Royal Astronomical Society, 1997
- Three New “51 Pegasi–Type” PlanetsThe Astrophysical Journal, 1997
- Properties of Sun-like Stars with Planets: [CLC]ρ[TSUP]1[/TSUP][/CLC] Cancri, τ Bootis, and υ AndromedaeThe Astrophysical Journal, 1997
- A Jupiter-mass companion to a solar-type starNature, 1995
- The starpatch on the G8 dwarf XI Bootis AThe Astrophysical Journal, 1988
- Observational evidence against differential rotation in F starsThe Astrophysical Journal, 1982