Light and velocity curves of bump Cepheids
Conference
·
OSTI ID:6225882
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.
- Research Organization:
- Los Alamos National Lab., NM (USA)
- DOE Contract Number:
- W-7405-ENG-36
- OSTI ID:
- 6225882
- Report Number(s):
- LA-UR-85-4110; CONF-8510265-3; ON: DE86003651
- Country of Publication:
- United States
- Language:
- English
Similar Records
Light curves for ''bump Cepheids'' computed with a dynamically zoned pulsation code
Light and velocity curve bumps for BW Vulpeculae
Theoretical study of Cepheid light curves
Conference
·
Sat Dec 31 23:00:00 EST 1977
·
OSTI ID:6604873
Light and velocity curve bumps for BW Vulpeculae
Conference
·
Mon Dec 31 23:00:00 EST 1979
·
OSTI ID:6790403
Theoretical study of Cepheid light curves
Conference
·
Tue May 01 00:00:00 EDT 1984
·
OSTI ID:6805973
Related Subjects
640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CEPHEIDS
DATA
INFORMATION
LUMINOSITY
MATHEMATICAL MODELS
NUMERICAL DATA
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
PULSATING VARIABLE STARS
PULSATIONS
STAR MODELS
STARS
THEORETICAL DATA
TIME DEPENDENCE
VARIABLE STARS
VARIATIONS
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CEPHEIDS
DATA
INFORMATION
LUMINOSITY
MATHEMATICAL MODELS
NUMERICAL DATA
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
PULSATING VARIABLE STARS
PULSATIONS
STAR MODELS
STARS
THEORETICAL DATA
TIME DEPENDENCE
VARIABLE STARS
VARIATIONS