LUMINOSITY OF VERY RED SUPERGIANT NEAR CLUSTER TR 27

被引：7

作者：

IMHOFF, CL

KEENAN, PC

机构：

[1] PERKINS OBSERV,DELAWARE,OH 43015

[2] OHIO WESLEYAN UNIV,DELAWARE,OH

来源：

ASTROPHYSICAL JOURNAL | 1976年 / 205卷 / 02期

关键词：

D O I：

10.1086/154298

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：455 / &

共 10 条

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[2]

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[3]

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[4] M SUPERGIANTS IN PERSEUS ARM [J].

HUMPHREYS, RW .

ASTROPHYSICAL JOURNAL, 1970, 160 (03) :1149-+

[5] WIDTH OF HALPHA AS DISCRIMINANT OF LUMINOSITY IN SPECTRA OF LATE-TYPE STARS [J].

KRAFT, RP ;

PRESTON, GW ;

WOLFF, SC .

ASTROPHYSICAL JOURNAL, 1964, 140 (01) :235-&

[6] PHOTOMETRY OF HIGH-LUMINOSITY M-TYPE STARS [J].

LEE, TA .

ASTROPHYSICAL JOURNAL, 1970, 162 (01) :217-&

[7] SPECTRAL CLASSIFICATION [J].

MORGAN, WW ;

KEENAN, PC .

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1973, 11 :29-50

[8]

Roman N. G., 1973, SPECTRAL CLASSIFICAT, P36

[9]

THE PS, 1970, ASTRON ASTROPHYS, V5, P298

[10]

WHITE NM, 1971, THESIS OHIO STATE U

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