INFRARED OBSERVATIONS OF THE Z=3.8 RADIO GALAXY, 4C 41.17, WITH THE KECK,W.M. TELESCOPE

被引:40
作者
GRAHAM, JR
MATTHEWS, K
SOIFER, BT
NELSON, JE
HARRISON, W
JERNIGAN, JG
LIN, S
NEUGEBAUER, G
SMITH, G
ZIOMKOWSKI, C
机构
[1] CALTECH,PALOMAR OBSERV,PASADENA,CA 91125
[2] CALIF ASSOC RES ASTRON,KAMUELA,HI 96743
[3] UNIV CALIF BERKELEY,SPACE SCI LAB,BERKELEY,CA 94720
关键词
EARLY UNIVERSE; GALAXIES; ACTIVE; FORMATION; RADIO CONTINUUM;
D O I
10.1086/187149
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The near-infrared camera on the W. M. Keck telescope has been used to image the z = 3.8 radio galaxy 4C 41.17. The 2 mu m continuum consists of a thin ace of emission aligned along the radio axis. There is close correlation between the optical, infrared, and radio emission. The color of 4C 41.17 is blue (R-K-s, = 2.7 +/- 0.1 mag). This may indicate ongoing star formation, but the origin of the continuum emission remains unclear. [OIII] and H beta emission makes a large contribution to the K-band flux. A number of faint red companions of 4C 41.17 are detected in the 2 mu m image. If these sources are at the same redshift as 4C 41.17, then their red colors indicate ages of more than similar to 0.5 Gyr and an epoch of formation at z greater than or similar to 8.
引用
收藏
页码:L5 / L8
页数:4
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