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Results: 1-4 |
Results: 4
THE RELATION BETWEEN THE INITIAL AND FINAL MASSES OF STARS WITH DIFFERENT CHEMICAL-COMPOSITIONS
Authors: FRANTSMAN YL PYLEVA NA
Citation: Yl. Frantsman et Na. Pyleva, THE RELATION BETWEEN THE INITIAL AND FINAL MASSES OF STARS WITH DIFFERENT CHEMICAL-COMPOSITIONS, Astronomy reports, 42(5), 1998, pp. 613-620
DIFFERENCES IN C O DISTRIBUTIONS OF CARBON STARS AS AN INDICATOR OF THE INHOMOGENEITY OF CHEMICAL-COMPOSITION IN THE GALAXY/
Authors: FRANTSMAN YL EGLITIS I PYLEVA NA
Citation: Yl. Frantsman et al., DIFFERENCES IN C O DISTRIBUTIONS OF CARBON STARS AS AN INDICATOR OF THE INHOMOGENEITY OF CHEMICAL-COMPOSITION IN THE GALAXY/, Astronomy reports, 42(2), 1998, pp. 193-199
HIGH-LUMINOSITY CARBON STARS IN THE EARLY ASYMPTOTIC GIANT BRANCH PHASE
Authors: FRANTSMAN YL PYLEVA NA
Citation: Yl. Frantsman et Na. Pyleva, HIGH-LUMINOSITY CARBON STARS IN THE EARLY ASYMPTOTIC GIANT BRANCH PHASE, ASTRONOM ZH, 72(6), 1995, pp. 841-847
THE ORIGIN OF CARBON STARS WITH HIGH C O IN THE ATMOSPHERES/
Authors: FRANTSMAN YL EGLITIS IE
Citation: Yl. Frantsman et Ie. Eglitis, THE ORIGIN OF CARBON STARS WITH HIGH C O IN THE ATMOSPHERES/, ASTRONOM ZH, 70(6), 1993, pp. 1228-1236
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