Journal
ASTRONOMICAL JOURNAL
Volume 144, Issue 1, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/144/1/19
Keywords
planetary systems; stars: individual (HAT-P-34, GSC 1622-01261, HAT-P-35, GSC 0203-01079, HAT-P-36, ... ...); techniques: photometric; techniques: spectroscopic
Categories
Funding
- NASA [NNG04GN74G, NNX08AF23G]
- NSF [AST-1108686]
- Kepler Mission under NASA [NCC2-1390]
- Hungarian Scientific Research Foundation (OTKA) [K-81373]
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1108686] Funding Source: National Science Foundation
Ask authors/readers for more resources
We report the discovery of four transiting extrasolar planets (HAT-P-34b-HAT-P-37b) with masses ranging from 1.05 to 3.33 M-J and periods from 1.33 to 5.45 days. These planets orbit relatively bright F and G dwarf stars (from V = 10.16 to V = 13.2). Of particular interest is HAT-P-34b which is moderately massive (3.33 M-J), has a high eccentricity of e = 0.441 +/- 0.032 at a period of P = 5.452654 +/- 0.000016 days, and shows hints of an outer component. The other three planets have properties that are typical of hot Jupiters.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available