THE CHEMICAL-COMPOSITION OF THE COOL WHITE-DWARF LP-701-29

被引：13

作者：

KAPRANIDIS, S ^{[1
]}

LIEBERT, J ^{[1
]}

机构：

[1] WASHBURN UNIV,DEPT MATH,TOPEKA,KS 66621

来源：

ASTROPHYSICAL JOURNAL | 1986年 / 305卷 / 02期

关键词：

D O I：

10.1086/164300

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：863 / 866

页数：4

共 26 条

[1]

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BESSELL, MS ;

WICKRAMASINGHE, DT .

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[3] LP 701-29 - NEW LOWEST LUMINOSITY DEGENERATE STAR WITH A HEAVILY BLANKETED SPECTRUM [J].

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HINTZEN, PM ;

LIEBERT, JW ;

STOCKMAN, HS ;

SPINRAD, H .

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[4]

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[5]

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[6]

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[7] THE FREQUENCY OF HYDROGEN WHITE-DWARFS AS OBSERVED AT HIGH SIGNAL TO NOISE RATIO [J].

GREENSTEIN, JL .

ASTROPHYSICAL JOURNAL, 1986, 304 (01) :334-355

[8] EMERGING MONOCHROMATIC FLUXES AND COLORS OF RED DEGENERATE STARS [J].

KAPRANIDIS, S .

ASTROPHYSICAL JOURNAL, 1985, 294 (02) :634-639

[9] MODEL ATMOSPHERES OF RED DEGENERATE STARS [J].

KAPRANIDIS, S .

ASTROPHYSICAL JOURNAL, 1983, 275 (01) :342-353

[10]

KOESTER D, 1976, ASTRON ASTROPHYS, V52, P415

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