Evidence for non-radiative activity in hot stars

Details Evidence for non-radiative activity in hot stars Evidence for non-radiative activity in hot stars

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358....2c&link_type=abstract

In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 2-23 (SEE N85-17755 08-88)

Physics

1

Early Stars, Hot Stars, Infrared Radiation, Luminosity, Radiative Transfer, Solar Corona, Stellar Atmospheres, Stellar Rotation, Stellar Temperature, X Ray Sources, X Ray Spectra

Scientific paper

Indications of non-radiative activity in hot stars were investigated. Data used as evidence of non-radiative activity includes: (1) evidence for high temperature regions, especially regions that are too hot to be explained by shocks that can be initiated and driven by radiative forces; (2) evidence for multi-plume flow. Non-spherically symmetric flow can be diagnosed by the effect it can have on the polarization of the light from a star; and (3) direct evidence for stellar magnetic fields.

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