scholarly journals A Mass Function Constraint on Extrasolar Giant Planet Evaporation Rates

2007 ◽  
Vol 658 (1) ◽  
pp. L59-L62 ◽  
Author(s):  
W. B. Hubbard ◽  
M. F. Hattori ◽  
A. Burrows ◽  
I. Hubeny
2008 ◽  
Vol 390 (3) ◽  
pp. 1258-1266 ◽  
Author(s):  
J. R. Barnes ◽  
Travis S. Barman ◽  
H. R. A. Jones ◽  
C. J. Leigh ◽  
A. Collier Cameron ◽  
...  

2001 ◽  
Vol 560 (1) ◽  
pp. 413-419 ◽  
Author(s):  
W. B. Hubbard ◽  
J. J. Fortney ◽  
J. I. Lunine ◽  
A. Burrows ◽  
D. Sudarsky ◽  
...  

2004 ◽  
Vol 202 ◽  
pp. 269-276
Author(s):  
Mark S. Marley ◽  
Andrew S. Ackerman

Clouds and hazes are important throughout our solar system and in the atmospheres of brown dwarfs and extrasolar giant planets. Among the brown dwarfs, clouds control the colors and spectra of the L-dwarfs; the disappearance of clouds helps herald the arrival of the T-dwarfs. The structure and composition of clouds will be among the first remote-sensing results from the direct detection of extrasolar giant planets.


Nature ◽  
2005 ◽  
Vol 436 (7048) ◽  
pp. 230-233 ◽  
Author(s):  
Maciej Konacki

2010 ◽  
Vol 722 (1) ◽  
pp. 178-187 ◽  
Author(s):  
Tommi T. Koskinen ◽  
James Y-K. Cho ◽  
Nicholas Achilleos ◽  
Alan D. Aylward

2008 ◽  
Author(s):  
Russell B. Makidon ◽  
Anand Sivaramakrishnan ◽  
Rémi Soummer ◽  
Jay Anderson ◽  
Roeland P. van der Marel

2004 ◽  
Vol 202 ◽  
pp. 12-19 ◽  
Author(s):  
S. Udry ◽  
M. Mayor ◽  
D. Queloz

6 new extra-solar planet candidates (HD 6434 b, HD 19994 b, HD 83443c, HD 92788b, HD 121504b, HD 190228b) are announced as part of our planet-search programmes in the northern and southern hemispheres. HD 83443 c is member of a 2-planet system with Saturnian and sub-Saturnian masses. Another system including a planet + a very low-mass brown dwarf orbiting HD 168443 is also presented. These 2 new systems and the new planetary detections rise to 25 the number of ELODIE and CORALIE candidates with minimum masses ≤20MJup. The orbital element distributions of giant-planet candidates, like the secondary mass function, the eccentricity and period distributions, compared to the equivalent distributions for spectroscopic binaries, strongly suggest different formation mechanisms for the two populations.


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