INTENSITY OF INTER-STELLAR LYMAN ALPHA

被引：11

作者：

DRAINE, BT ^{[1
]}

SALPETER, EE ^{[1
]}

机构：

[1] CORNELL UNIV,CTR RADIOPHYS & SPACE RES,ITHACA,NY 14853

来源：

NATURE | 1978年 / 271卷 / 5647期

关键词：

D O I：

10.1038/271730a0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

引用

页码：730 / 731

页数：2

共 17 条

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[2]

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[4] ENERGY PER ION PAIR FOR ELECTRON AND PROTON BEAMS IN ATOMIC HYDROGEN [J].

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[5]

DRAINE BT, ASTROPHYS J SUPPL

[6] ISOLATED STROMGREN SPHERES AS A SOURCE OF GALACTIC HALPHA EMISSION [J].

ELMERGREEN, BG .

ASTROPHYSICAL JOURNAL, 1975, 198 (01) :L31-L35

[7]

FALGARONE E, 1973, ASTRON ASTROPHYS, V25, P253

[8] FORMATION AND DESTRUCTION RATES OF INTERSTELLAR H2 [J].

JURA, M .

ASTROPHYSICAL JOURNAL, 1974, 191 (02) :375-379

[9] ULTRAVIOLET PHOTOMETRY FROM ORBITING ASTRONOMICAL OBSERVATORY .25. DIFFUSE GALACTIC LIGHT IN 1500-4200 A REGION AND SCATTERING PROPERTIES OF INTERSTELLAR DUST GRAINS [J].

LILLIE, CF ;

WITT, AN .

ASTROPHYSICAL JOURNAL, 1976, 208 (01) :64-74

[10] NUMERICAL-MODELS FOR SUPERNOVA-REMNANTS [J].

MANSFIELD, VN ;

SALPETER, EE .

ASTROPHYSICAL JOURNAL, 1974, 190 (02) :305-313

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