Published September 1980 | Version v1
Journal article

Three-mode resonances in double-mode cepheids

  • 1. Sussex Univ., Brighton (UK). Astronomy Centre
  • 2. Tohoku Univ., Sendai (Japan). Faculty of Science

Description

The three-wave resonances are studied for models with helium enriched inhomogeneous outer layers. The resonance among the fundamental mode, the first overtone, and the third overtone is studied for several models with Ysub(S) = 0.5 and Zsub(S)/Xsub(S) = 0.02/0.70. The model having the evolutionary mass cannot give both the observed period ratio and a sufficiently strong resonance. Masses less than the evolutionary mass or with more enriched helium abundance for the outermost layers are needed to explain the observation. (author)

Additional details

Publishing Information

Journal Title
Mon. Not. R. Astron. Soc.
Journal Volume
192
Journal Issue
3
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
697-707
ISSN
0035-8711

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
11567582
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CEPHEIDS; ELEMENT ABUNDANCE; HELIUM; MASS; OSCILLATION MODES; RESONANCE; STAR EVOLUTION; STAR MODELS
Descriptors DEC
ELEMENTS; MATHEMATICAL MODELS; NONMETALS; PULSATING VARIABLE STARS; QUANTITY RATIO; RARE GASES; STARS; VARIABLE STARS