The Rossiter-McLaughlin effect of CoRoT-3b & HD189733b

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

7 pages, 4 figures, accepted in A&A for publication

Scientific paper

We present radial-velocity sequences acquired during three transits of the exoplanet HD 189733b and one transit of the CoRoT-3b. We applied a combined Markov-Chain Monte Carlo analysis of spectroscopic and photometric data on these stars, to determine a full set of system parameters including the project spin-orbit misalignement angle of HD 189733b to an unprecedented precision via the Rossiter-McLaughlin effect: beta = 0.85 degrees (+0.32 -0.28) . This small but non-zero inclination of the planetary orbit is important to understand the origin of the system. On CoRoT-3b, results seem to point towards a non-zero inclination as well with beta = 37.6 degrees (+10.0 -22.3), but this remains marginal. Systematic effects due to non-gaussian cross-correlation functions appear to be the main cause of significant residuals that prevent an accurate determination of the projected stellar rotation velocity V sin(I) for both stars.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The Rossiter-McLaughlin effect of CoRoT-3b & HD189733b 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 The Rossiter-McLaughlin effect of CoRoT-3b & HD189733b, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Rossiter-McLaughlin effect of CoRoT-3b & HD189733b will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-109912

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.