The magnetic field of the planet-hosting star τ Bootis
Open Access
- 1 January 2007
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society: Letters
- Vol. 374 (1) , L42-L46
- https://doi.org/10.1111/j.1745-3933.2006.00261.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 21 references indexed in Scilit:
- The surprising magnetic topology of Sco: fossil remnant or dynamo output?Monthly Notices of the Royal Astronomical Society, 2006
- The Large-Scale Axisymmetric Magnetic Topology of a Very-Low-Mass Fully Convective StarScience, 2006
- Tomographic studies of exoplanet atmospheresAstronomische Nachrichten, 2004
- Dynamo processes and activity cycles of the active stars AB Doradus, LQ Hydrae and HR 1099Monthly Notices of the Royal Astronomical Society, 2003
- A False Planet around HD 192263The Astrophysical Journal, 2002
- The global magnetic topology of AB DoradusMonthly Notices of the Royal Astronomical Society, 2002
- On Stellar Activity Enhancement Due to Interactions with Extrasolar Giant PlanetsThe Astrophysical Journal, 2000
- Photometric and CaiiH and K Spectroscopic Variations in Nearby Sun‐like Stars with Planets. III.The Astrophysical Journal, 2000
- Spectropolarimetric observations of active starsMonthly Notices of the Royal Astronomical Society, 1997
- Three New “51 Pegasi–Type” PlanetsThe Astrophysical Journal, 1997