WAVELENGTH SHIFTS AND PROBABLE ISOTOPIC STRUCTURE OF PT II LAMBDA-4046 IN MERCURY STARS

被引：40

作者：

DWORETSK.MM ^{[1
]}

VAUGHAN, AH ^{[1
]}

机构：

[1] HALE OBSERV,PASADENA,CA 91109

来源：

关键词：

D O I：

10.1086/152092

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：811 / 816

页数：6

共 13 条

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[4] ORBIT OF DOUBLE-LINED BINARY MERCURY STAR CHI-LUPI [J].

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[5]

DWORETSKY MM, 1971, B AAS, V3, P350

[6]

GUTHRIE BNG, 1969, OBSERVATORY, V89, P224

[7]

MOORE CE, 1958, NBS467 CIRC

PRESTON, GW .

[9] RELATIVE ISOTOPIC ABUNDANCES OF MERCURY IN MERCURY STARS [J].

PRESTON, GW ;

VAUGHAN, AH ;

WHITE, RE ;

SWINGS, JP .

[10]

PRESTON GW, IN PRESS