Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009a%26a...499..623d&link_type=abstract
Astronomy and Astrophysics, Volume 499, Issue 2, 2009, pp.623-625
Astronomy and Astrophysics
Astrophysics
1
Techniques: Radial Velocities, Stars: Early-Type, Stars: Planetary Systems, Stars: Oscillations, Individual: Hd 60532, Errata, Addenda
Scientific paper
The dynamical analysis in the original paper was erroneous due to a mismatch in the choice of angular parameters. The calculations had been made by assuming a pole-on (sin i = 0) instead of an edge-on sin i = 1 orbit. In this framework, Ω_c-Ωb is just the mutual inclination between the orbital planes of the two planets. We also correct some stellar parameters given in the original paper (log g = +3.83, [Fe/H]updated = -0.26 ).
Beust Hervé
Desort Morgan
Galland Franck
Lagrange Anne Marie
Lo Curto Gaspare
No associations
LandOfFree
Extrasolar planets and brown dwarfs around A-F type stars. V. A planetary system found with HARPS around the F6IV-V star HD 60532 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Extrasolar planets and brown dwarfs around A-F type stars. V. A planetary system found with HARPS around the F6IV-V star HD 60532, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Extrasolar planets and brown dwarfs around A-F type stars. V. A planetary system found with HARPS around the F6IV-V star HD 60532 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1105576