CORE MASS-INTERFLASH PERIOD RELATION FOR DOUBLE SHELL SOURCE STARS

被引：80

作者：

PACZYNSKI, B

机构：

[1] POLISH ACAD SCI,INST ASTRON,AL UJAZDOWSKIE 4,00-478 WARSAW,POLAND

[2] PRINCETON UNIV OBSERV,PRINCETON,NJ

来源：

关键词：

D O I：

10.1086/154006

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：558 / 560

页数：3

共 17 条

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[2] CHRISTYSACKMANN IJ, 1974, 19TH LIEG COLL
[3] FLANNERY BP, 1973, ASTROPHYS J, V183, P491, DOI 10.1086/152241
[4] THERMAL PULSES - P-CAPTURE, ALPHA-CAPTURE, S-PROCESS NUCLEOSYNTHESIS - CONVECTIVE MIXING IN A STAR OF INTERMEDIATE MASS
IBEN, I
[J]. ASTROPHYSICAL JOURNAL, 1975, 196 (02) : 525 - 547
[5] FG SAGITTAE - S-PROCESS EPISODE
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ANDERSON, KS
[J]. ASTROPHYSICAL JOURNAL, 1974, 189 (03) : 509 - 521
[6] Paczynski B., 1970, Acta Astronomica, V20, P287
[7] Paczynski B., 1970, Acta Astronomica, V20, P47
[8] HELIUM-SHELL FLASHES IN POPULATION I STARS
PACZYNSKI, B
[J]. ASTROPHYSICAL JOURNAL, 1974, 192 (02) : 483 - 485
[9] Paczynski B., 1971, Acta Astronomica, V21, P271
[10] PACZYNSKI B, UNPUBLISHED DATA