THE BELL-LABORATORIES H-I SURVEY

被引:1139
作者
STARK, AA
GAMMIE, CF
WILSON, RW
BALLY, J
LINKE, RA
HEILES, C
HURWITZ, M
机构
[1] AT&T BELL LABS,RADIO PHYS RES DEPT,HOLMDEL,NJ 07733
[2] UNIV CALIF BERKELEY,BERKELEY,CA 94720
关键词
ISM; GENERAL; RADIO LINES; ATOMIC; SURVEYS;
D O I
10.1086/191645
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The sky north of delta = -40-degrees was observed in the 21 cm line of atomic hydrogen with the FWHM = 2-degrees beam of the 20 foot horn reflector at AT&T Bell Laboratories, Crawford Hill. The survey covers a velocity range of 654 km s-1 centered on the Galactic standard of rest, with 5.3 km s-1 wide filters. Calibration and reduction of the observations are described. The survey is presented as a series of images of the sky, each covering a 10 km s-1 wide velocity range. This survey is distinguished by its sensitivity to low surface brightness features (T(A) almost-equal-to 50 mK) and relative freedom from sidelobe contamination. High-velocity clouds are extracted and cataloged automatically. At the resolution of the survey, the lowest H I column density in the sky is 5.7 x 10(19) cm-2.
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页码:77 / &
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