Derivation of the Rotational Frequency of Massive Stars from Seismic Studies

Details Derivation of the Rotational Frequency of Massive Stars from Seismic Studies Derivation of the Rotational Frequency of Massive Stars from Seismic Studies

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..215..199a&link_type=gif

Stellar Rotation, Proceedings of IAU Symposium No. 215, held 11-15 November, 2002 in Cancun, Yucatan, Mexico. Edited by Andre M

Astronomy and Astrophysics

Astronomy

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