NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login
Back to Results
Non-radiative Energy from Differential Rotation in Hot StarsA 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.
Document ID
19850009469
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Chan, K. L. (Applied Research Corp. Landover, Md., United States)
Mayr, H. G. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Harris, I. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1985
Publication Information
Publication: The Origin of Nonradiative Heating(Momentum in Hot Stars
Subject Category
Astrophysics
Accession Number
85N17778
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
Document Inquiry

Available Downloads

There are no available downloads for this record.

Related Records

IDRelationTitle19850009446Collected WorksThe Origin of Nonradiative Heating/momentum in Hot Stars
No Preview Available