The Rossiter-McLaughlin Rotation Effect for HD 209458 Due to a Planetary Transit

Details The Rossiter-McLaughlin Rotation Effect for HD 209458 Due to a Planetary Transit The Rossiter-McLaughlin Rotation Effect for HD 209458 Due to a Planetary Transit

Jan 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ibvs.4838....1w&link_type=abstract

Information Bulletin on Variable Stars, 4838, 1.

Physics

3

Scientific paper

The transit of a planet across the disk of HD209458 has recently been
photometrically detected. An attempt should now be made to observe the
Rossiter-McLaughlin rotation effect in this star's radial-velocity curve

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