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1 edition of Origin of nonradiative heating/momentum in hot stars found in the catalog.

Origin of nonradiative heating/momentum in hot stars

Origin of nonradiative heating/momentum in hot stars

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Published by NASA, Scientific and Technical Information Branch in [Washington, D.C.] .
Written in English


Edition Notes

Statementedited by A. B. Underhill and A. G. Michalitsianos.
SeriesNASA Conference publication -- 2358
ID Numbers
Open LibraryOL14866939M

  HOT WHITE DWARF SHINES IN YOUNG STAR CLUSTER. NASA Technical Reports Server (NTRS) A dazzling 'jewel-box' collection of o stars .   The Origin of Nonradiative Heating/momentum in Hot Stars. NASA Technical Reports Server (NTRS) Underhill, A. B. (Editor); Michalitsianos, A. G. (Editor) The origin of nonradiative heating and momentum in the atmospheres of stars is studied.

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Origin of nonradiative heating/momentum in hot stars Download PDF EPUB FB2

Get this from a library. The Origin of nonradiative heating/momentum in hot stars. [Anne Barbara Underhill; A G Michalitsianos; Goddard Space Flight Center.; United States. National Aeronautics and Space Administration,; American Astronomical Society.;]. The Origin of Nonradiative Heating/Momentum in Hot Stars [Underhill, A.B.

And Michalitsianos, A.G.] on *FREE* shipping on qualifying offers. The Origin of Nonradiative Heating/Momentum in Hot StarsAuthor: A.G. Underhill, A.B. And Michalitsianos. Get this from a library. The Origin of nonradiative heating/momentum in hot stars: proceedings of a workshop sponsored by the National Aeronautics and Space Administration, Washington, D.C., and the American Astronomical Society, Washington, D.C., and held at NASA Goddard Space Flight Center, Greenbelt, Maryland, June[Anne Barbara Underhill; A G Michalitsianos; United States.

Nonradiative heating in the atmospheres of stars and the deposit of nonradiative momentum in the stellar atmosphere were examined. Observations made from space have been very important in changing the concept of what a star is like.

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A model of differential rotation is proposed for the upper radiative envelopes of hot stars, and it is suggested that the actions of such motions can be the source of energy for heating the coronae. The Origin of nonradiative heating/momentum in hot stars: proceedings of a workshop sponsored by the National Aeronautics and Space Administration, Washington, D.C., and the American Astronomical Society, Washington, D.C., and held at NASA Goddard Space Flight Center, Greenbelt, Maryland, June/ ([Washington, D.C.]: National.

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