FAR-INFRARED LINE AND CONTINUUM OBSERVATIONS OF G0.095+0.012 AND THE E2 THERMAL RADIO FILAMENT NEAR THE GALACTIC-CENTER

被引：31

作者：

ERICKSON, EF

COLGAN, SWJ

SIMPSON, JP

RUBIN, RH

MORRIS, M

HAAS, MR

机构：

[1] UNIV CALIF BERKELEY,SETI INST,BERKELEY,CA 94720

[2] UNIV CALIF LOS ANGELES,DEPT ASTRON,156205,8979 MATH SCI BLDG,LOS ANGELES,CA 90024

[3] UNIV CALIF BERKELEY,DEPT ASTRON,BERKELEY,CA 94720

来源：

ASTROPHYSICAL JOURNAL | 1991年 / 370卷 / 02期

关键词：

GALAXIES; NUCLEI; THE GALAXY; INFRARED; SOURCES;

D O I：

10.1086/185979

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Measurements of far-infrared lines and continuum from G0.095 + 0.012 and the E2 thermal "arched" radio filament near the Galactic center are well explained by numerous embedded stars with T(eff) approximately 35,000 K. The structure of the filament and the apparent absence of hotter stars are qualitatively difficult to reconcile with this idea.

引用

页码：L69 / &

共 31 条

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