EXTINCT RADIOACTIVITIES - A 3-PHASE MIXING MODEL

被引：35

作者：

CLAYTON, DD ^{[1
]}

机构：

[1] MAX PLANCK INST NUCL PHYS,D-6900 HEIDELBERG,FED REP GER

来源：

关键词：

D O I：

10.1086/160962

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：381 / 384

页数：4

共 18 条

[11] MASS-SPECTRUM OF INTER-STELLAR CLOUDS
KWAN, J
[J]. ASTROPHYSICAL JOURNAL, 1979, 229 (02) : 567 - 577
[12] AL-26 IN EARLY SOLAR-SYSTEM - FOSSIL OR FUEL
LEE, T
PAPANASTASSIOU, DA
WASSERBURG, GJ
[J]. ASTROPHYSICAL JOURNAL, 1977, 211 (02) : L107 - L110
[13] THEORY OF INTERSTELLAR-MEDIUM - 3 COMPONENTS REGULATED BY SUPERNOVA EXPLOSIONS IN AN INHOMOGENEOUS SUBSTRATE
MCKEE, CF
OSTRIKER, JP
[J]. ASTROPHYSICAL JOURNAL, 1977, 218 (01) : 148 - 169
[14] REEVES H, 1972, ORIGIN SOLAR SYSTEM
[15] SCHRAMM DN, 1973, SPACE SCI REV, V15, P51, DOI 10.1007/BF00172436
[16] Spitzer L, 1978, PHYS PROCESSES INTER
[17] Townes C. H., 1977, Topics in Intersteller Matter, P113
[18] NUCLEAR CHRONOLOGIES FOR GALAXY
WASSERBURG, GJ
SCHRAMM, DN
HUNEKE, JC
[J]. ASTROPHYSICAL JOURNAL, 1969, 157 (2P2) : L91 - +