THE INFRARED-EMISSION OF G333.6-0.2, AN EXTREMELY NONSPHERICAL H-II REGION

被引：28

作者：

HYLAND, AR

MCGREGOR, PJ

ROBINSON, G

THOMAS, JA

BECKLIN, EE

GATLEY, I

WERNER, MW

机构：

[1] CALTECH,DIV PHYS MATH & ASTRON,PASADENA,CA 91109

[2] UNIV MELBOURNE,RAAF ACAD,SCH PHYS,PARKVILLE,VIC 3052,AUSTRALIA

来源：

ASTROPHYSICAL JOURNAL | 1980年 / 241卷 / 02期

关键词：

D O I：

10.1086/158381

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：709 / 718

页数：10

共 41 条

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[3] ACCRETION POWERS THE BRIGHTEST STARS [J].

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WERNER, MW .

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[5] H II REGION G333.6-0.2 - VERY POWERFUL 1-20 MICRON SOURCE [J].

BECKLIN, EE ;

FROGEL, JA ;

NEUGEBAUER, G ;

PERSSON, SE ;

WYNNWILL.CG .

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[6]

CHEUNG L, 1980, PREPRINT

[7] NEBULOSITY ASSOCIATED WITH POWERFUL INFRARED AND RADIO-SOURCE G333.6-0.2 [J].

CHURMS, J ;

FEAST, MW ;

GLASS, IS ;

HARDING, GA ;

EVANS, TL ;

MARTIN, WL .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1974, 169 (02) :P39-&

[8]

CONTI PS, 1975, ASTRON ASTROPHYS, V38, P467

[9] 40-350 MICRON OBSERVATIONS OF GALACTIC SOURCES [J].

FURNISS, I ;

JENNINGS, RE ;

MOORWOOD, AFM .

ASTROPHYSICAL JOURNAL, 1975, 202 (02) :400-406

[10]

FURNISS I, 1974, REGIONS GALACTIC CTR, P61

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