Astrophysics, abstract
astro-ph/0605670
From: Alessandro Sozzetti [view email]
Date: Fri, 26 May 2006 15:56:31 GMT (177kb)
A Keck/HIRES Doppler Search for Planets Orbiting Metal-Poor Dwarfs. I. Testing Giant Planet Formation and Migration Scenarios
Authors: A. Sozzetti (1,2), G. Torres (1), D.W. Latham (1), B.W. Carney (3), R.P. Stefanik (1), A.P. Boss (4), J.B. Laird (5), S.G. Korzennik (1) ((1) Harvard-Smithsonian Center for Astrophysics, (2) INAF - Osservatorio Astronomico di Torino, (3) University of North Carolina, (4) Carnegie Institution of Washington, (5) Bowling Green State University)
Comments: 25 pages, 7 figures, accepted for publication in the Astrophysical Journal
We describe a high-precision Doppler search for giant planets orbiting a well-defined sample of metal-poor dwarfs in the field. This experiment constitutes a fundamental test of theoretical predictions which will help discriminate between proposed giant planet formation and migration models. We present here details on the survey as well as an overall assessment of the quality of our measurements, making use of the results for the stars that show no significant velocity variation.
http://arxiv.org/abs/astro-ph/0605670
Space/Science » in reply to No Detectable H3+ Emission from the Atmospheres of Hot Jupiters
A Keck/HIRES Doppler Search for Planets Orbiting Metal-Poor Dwarfs. I. Testing Giant Planet Formation and Migration Scenarios
The whole thread (9 posts)
- No Detectable H3+ Emission from the Atmospheres of Hot Jupiters
- A Keck/HIRES Doppler Search for Planets Orbiting Metal-Poor Dwarfs. I. Testing Giant Planet Formation and Migration Scenarios
- Toroidal Atmospheres around Extrasolar Planets
- Accretion Disks around Young Stars: Lifetimes, Disk Locking and Variability
- Toroidal Atmospheres around Extrasolar Planets
- A Keck/HIRES Doppler Search for Planets Orbiting Metal-Poor Dwarfs. I. Testing Giant Planet Formation and Migration Scenarios
