Computer Science
Scientific paper
Dec 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286...99d&link_type=abstract
In ESA, Seismology of the Sun and Sun-Like Stars p 99-102 (SEE N89-25819 19-92)
Computer Science
7
Solar Rotation, Subgiant Stars, Sun, Angular Momentum, Helioseismology, P Waves
Scientific paper
Attention is drawn to observations of surface rotational bands in subgiants which indicate that a deep-seated reservoir of angular momentum must exist in these stars. This interpretation is compatible with theoretical studies of the rotational history of the Sun and Sun-like stars, but is in conflict with observations of p-mode splittings in the Sun. In order to understand better the source of this discrepancy, the predicted rotational splittings of several test rotation curves are compared to solar data.
Demarque Pierre
Guenther David B.
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