Rotational Splittings with CoRoT, Expected Number of Detections and Measurement Accuracy

Details Rotational Splittings with CoRoT, Expected Number of Detections and Measurement Accuracy Rotational Splittings with CoRoT, Expected Number of Detections and Measurement Accuracy

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006esasp1306..453g&link_type=abstract

"Proceedings of "The CoRoT Mission Pre-Launch Status - Stellar Seismology and Planet Finding" (ESA SP-1306). Editors: M. Fridlun

Physics

Scientific paper

One of the main goal of the CoRoT experiment is to determine the internal rotation of stars. A seismic measure of rotation requires the detection and an accurate measurement of rotational splittings. Our ability to achieve this goal with CoRoT observations depends on the properties of the target star (in short: spectral type and distance) and will be discussed.

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