Spectroscopic and interferometric approach for differential rotation in massive fast rotators

Details Spectroscopic and interferometric approach for differential rotation in massive fast rotators Spectroscopic and interferometric approach for differential rotation in massive fast rotators

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..103z&link_type=abstract

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU

Astronomy and Astrophysics

Astronomy

1

Stars: Rotation, Techniques: Spectroscopic, Techniques: Interferometric

Scientific paper

The coupling between the convective region in the envelope and rotation
can produce a surface latitudinal differential rotation that may induce
changes of the stellar geometry and on the spectral line profiles that
it may be scrutinized spectroscopically and by interferometry.

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