YOUNG STELLAR OBJECTS DETECTED BY IRAS

被引:40
|
作者
CLARK, FO
机构
[1] Geophysics Laboratory, (AFSC)/OPC, Hanscom AF Base
来源
关键词
INFRARED; SOURCES; SPECTROPHOTOMETRY; STARS; PRE-MAIN-SEQUENCE;
D O I
10.1086/191543
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Fluxes of 453 IRAS point sources selected for proximity to dense gas have been accurately determined by co-adding IRAS data. From this set, 258 sources are detected in all four bands: 12, 25, 60, and 100-mu-m. As distance from dense molecular material increases, these sources exhibit systematic trends in color and a markedly decreasing luminosity. These trends are broadly consistent with expected evolutionary changes in these stars, with younger objects found closer to dense gas. These data suggest a subtle variation on the criterion for identifying the youngest objects detectable by IRAS, in addition to that of steeply rising spectra: a color temperature which is uniform across all four IRAS bands in the range 40-50 K. These characteristics are used as a criterion to select point sources as candidate very young pre-main-sequence stars.
引用
收藏
页码:611 / 628
页数:18
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