NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login
Back to Results
Microturbulence and Wesselink radiiUsing the calibration of Bell and Parsons (1974), the effects of changes in microturbulence and surface gravity throughout the cycles of delta Cephei and eta Aquilae are estimated. When the changes in microturbulence are considered, Wesselink radii for these stars are reduced 20%.
Document ID
19800016749
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Evans, N. R. (Toronto Univ. Ontario)
Date Acquired
August 10, 2013
Publication Date
May 1, 1980
Publication Information
Publication: NASA. Goddard Space Flight Center Current Probl. in Stellar Pulsation Instabilities
Subject Category
Astrophysics
Accession Number
80N25242
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

Related Records

IDRelationTitle19800016736Collected WorksCurrent problems in Stellar Pulsation Instabilities
No Preview Available