HAT-P-32b AND HAT-P-33b: TWO HIGHLY INFLATED HOT JUPITERS TRANSITING HIGH-JITTER STARS
Authors:
- J. D. HartmanJHJ. D. Hartman
- Géza KovácsGKGéza Kovács
- A. W. HowardAHA. W. Howard
- D. A. FischerDFD. A. Fischer
- 3 November 2011
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 742 (1)
Abstract
No abstract availableAll Related Versions
This publication has 68 references indexed in Scilit:
- Thermal emission at 4.5 and 8 μm of WASP-17b, an extremely large planet in a slightly eccentric orbitMonthly Notices of the Royal Astronomical Society, 2011
- EVOLUTION OF OHMICALLY HEATED HOT JUPITERSThe Astrophysical Journal, 2011
- HAT-P-27b: A HOT JUPITER TRANSITING A G STAR ON A 3 DAY ORBITThe Astrophysical Journal, 2011
- INFLATING HOT JUPITERS WITH OHMIC DISSIPATIONThe Astrophysical Journal Letters, 2010
- HAT-P-11b: A SUPER-NEPTUNE PLANET TRANSITING A BRIGHT K STAR IN THEKEPLERFIELDThe Astrophysical Journal, 2010
- HD 147506b: A Supermassive Planet in an Eccentric Orbit Transiting a Bright StarThe Astrophysical Journal, 2007
- Possible Solutions to the Radius Anomalies of Transiting Giant PlanetsThe Astrophysical Journal, 2007
- Wide‐Field Millimagnitude Photometry with the HAT: A Tool for Extrasolar Planet DetectionPublications of the Astronomical Society of the Pacific, 2004
- On the Radii of Extrasolar Giant PlanetsThe Astrophysical Journal, 2003
- On the Tidal Inflation of Short‐Period Extrasolar PlanetsThe Astrophysical Journal, 2001