HIGH ANGULAR RESOLUTION BROAD-BAND IMAGING IN THE MIDINFRARED - THE INFRARED BRIGHT GALAXY NGC-34

被引:8
作者
KETO, E
JERNIGAN, G
BALL, R
ARENS, J
MEIXNER, M
机构
[1] UNIV HAWAII,NASA INFRARED TELESCOPE FACIL,HONOLULU,HI 96822
[2] UNIV CALIF BERKELEY,SPACE SCI LAB,BERKELEY,CA 94720
[3] UNIV CALIF LAWRENCE LIVERMORE NATL LAB,INST GEOPHYS & PLANETARY PHYS,LIVERMORE,CA 94550
[4] UNIV CALIF BERKELEY,DEPT ASTRON,BERKELEY,CA 94720
关键词
GALAXIES; GENERAL; INDIVIDUAL; (NGC-34);
D O I
10.1086/186064
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on a high angular resolution (1") mid-IR image of the IR-bright galaxy NGC 34. The observation shows the mid-IR emission to be very compact, less-than-or-equal-to 2.3" x 1.7" (less-than-or-equal-to 870 x 640 pc, D = 78 Mpc, H0 = 75 km s-1 Mpc-1). This and previous observations indicate sizes smaller than predicted by starburst models for the emission. The achieved sensitivity, 15 mJy minutes-1/2 arcsec-2, (1-sigma NEFD DELTA-lambda = 5-mu-m) is the highest sensitivity ever obtained for any observation with a mid-IR array camera.
引用
收藏
页码:L29 / L31
页数:3
相关论文
共 7 条
[1]  
CARICO DP, 1990, AJ, V100, P364
[2]  
KETO E, 1990, UNPUB APPL OPTICS
[3]  
RODRIGUESESPINA.JA, 1987, NASA CP2466, P669
[4]   MODELS FOR INFRARED-EMISSION FROM IRAS GALAXIES [J].
ROWANROBINSON, M ;
CRAWFORD, J .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1989, 238 (02) :523-558
[5]   THE IRAS BRIGHT GALAXY SAMPLE .2. THE SAMPLE AND LUMINOSITY FUNCTION [J].
SOIFER, BT ;
SANDERS, DB ;
MADORE, BF ;
NEUGEBAUER, G ;
DANIELSON, GE ;
ELIAS, JH ;
LONSDALE, CJ ;
RICE, WL .
ASTROPHYSICAL JOURNAL, 1987, 320 (01) :238-257
[6]  
VERONCETTY MP, 1989, CATALOG QUASARS ACTI
[7]  
WILSON AS, 1988, A A, V206, P14