Published 1985
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Light and velocity curves of bump Cepheids
Description
We present light and velocity curves for eight hydrodynamic bump Cepheid models. All of the models were converged to the fundamental mode solution using a relaxation technique developed by Stellingwerf (1974). Our use of this method assures that the time behavior repeats each period to better than one part in a thousand. The motivation for this work was to help Buchler, at the University of Florida, to develop his theory of modal interactions in pulsating stars. 4 refs., 8 figs
Availability note (English)
MF available from INIS under the Report Number; Available from NTIS, PC A02/MF A01; 1 as DE86003651.
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Additional details
Publishing Information
- Imprint Pagination
- 4 p.
- Report number
- LA-UR--85-4110
Conference
- Title
- 4. Cambridge workshop on cool stars, stellar systems, and the sun.
- Dates
- 16-18 Oct 1985.
- Place
- Santa Fe, NM (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 17056742
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference, Numerical Data
- Descriptors DEI
- CEPHEIDS; LUMINOSITY; PULSATIONS; STAR MODELS; THEORETICAL DATA; TIME DEPENDENCE; VARIATIONS
- Descriptors DEC
- DATA; INFORMATION; MATHEMATICAL MODELS; NUMERICAL DATA; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; PULSATING VARIABLE STARS; STARS; VARIABLE STARS
Optional Information
- Notes
- Portions of this document are illegible in microfiche products.
- Secondary number(s)
- CONF-8510265--3.