Differential Rotation in Solar-type Spectra

Details Differential Rotation in Solar-type Spectra Differential Rotation in Solar-type Spectra

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21443302b&link_type=abstract

American Astronomical Society, AAS Meeting #214, #433.02; Bulletin of the American Astronomical Society, Vol. 41, p.704

Astronomy and Astrophysics

Astronomy

Scientific paper

A continuing effort has developed a disk-integration model to study the effects of differential rotation and surface convection in the spectrum of sun-like stars (e.g., BAAS 38, 915, 2007; BAAS 40, 203, 2008). This poster extends the analysis to fast and slow rotators (previously limited v sin i from 2 to 6 km/s), a larger range in inclination, and non-solar convective line shifts. The pseudo-power spectrum is explored further as a diagnostic tool.

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