scholarly journals On the Tidal Interaction of a Solar‐Type Star with an Orbiting Companion: Excitation ofg‐Mode Oscillation and Orbital Evolution

1998 ◽  
Vol 502 (2) ◽  
pp. 788-801 ◽  
Author(s):  
C. Terquem ◽  
J. C. B. Papaloizou ◽  
R. P. Nelson ◽  
D. N. C. Lin
2008 ◽  
Vol 4 (T27A) ◽  
pp. 181-182
Author(s):  
Michel Mayor ◽  
Alan P. Boss ◽  
Paul R. Butler ◽  
William B. Hubbard ◽  
Philip A. Ianna ◽  
...  

Commission 53 on Extrasolar Planets was created at the 2006 Prague General Assembly of the IAU, in recognition of the outburst of astronomical progress in the field of extrasolar planet discovery, characterization, and theoretical work that has occurred since the discovery of the pulsar planets in 1992 and the discovery of the first planet in orbit around a solar-type star in 1995. Commission 53 is the logical successor to the IAU Working Group on Extrasolar Planets WG-ESP, which ended its six years of existence in August 2006. The founding president of Commission 53 is Michael Mayor, in honor of his seminal contributions to this new field of astronomy. The vice-president is Alan Boss, the former chair of the WG-ESP, and the members of the Commission 53 Organizing Committee are the other former members of the WG-ESP.


2005 ◽  
Vol 618 (2) ◽  
pp. 926-938 ◽  
Author(s):  
C. I. Short ◽  
P. H. Hauschildt
Keyword(s):  

2017 ◽  
Vol 605 ◽  
pp. A19 ◽  
Author(s):  
S. Orlando ◽  
F. Favata ◽  
G. Micela ◽  
S. Sciortino ◽  
A. Maggio ◽  
...  

2011 ◽  
Vol 731 (1) ◽  
pp. 69 ◽  
Author(s):  
Benjamin P. Brown ◽  
Mark S. Miesch ◽  
Matthew K. Browning ◽  
Allan Sacha Brun ◽  
Juri Toomre

2010 ◽  
Vol 518 ◽  
pp. A48 ◽  
Author(s):  
A. Frasca ◽  
K. Biazzo ◽  
Zs. Kővári ◽  
E. Marilli ◽  
Ö. Çakırlı

2015 ◽  
Vol 11 (S320) ◽  
pp. 224-229
Author(s):  
Dmitry V. Bisikalo ◽  
Alexander A. Cherenkov ◽  
Pavel V. Kaygorodov

AbstractWe consider the influence of a coronal mass ejection (CME) of a solar type star on the mass loss rate of a hot Jupiter exoplanet. We have conducted 3D numerical gas-dynamic simulations of the planet's atmosphere that interacts with CME. Using the results of these simulations we have estimated the specific parameters that influence the mass loss rate. Based on the assumption that CME totally sweeps away part of the planet's gaseous envelope located outside the Roche lobe we estimated the maximum mass loss rate. Finally, we have considered the dependence of mass loss rate on the frequency of CMEs in course of star's evolution.


Science ◽  
2017 ◽  
Vol 357 (6347) ◽  
pp. 159.1-159
Author(s):  
Keith T. Smith
Keyword(s):  
The Sun ◽  

2010 ◽  
Vol 724 (2) ◽  
pp. 866-877 ◽  
Author(s):  
G. Kovács ◽  
G. Á. Bakos ◽  
J. D. Hartman ◽  
G. Torres ◽  
R. W. Noyes ◽  
...  

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