A (CO)-C-12(1-0) survey of spiral galaxies in the region of the Coma supercluster

被引:27
作者
Casoli, F
Dickey, J
Kazes, I
Boselli, A
Gavazzi, G
Jore, K
机构
[1] ECOLE NORMALE SUPER,F-75231 PARIS 05,FRANCE
[2] UNIV MINNESOTA,DEPT ASTRON,MINNEAPOLIS,MN 55455
[3] OBSERV PARIS,MEUDON SECT,ARPEGES,F-92195 MEUDON,FRANCE
[4] MAX PLANCK INST KERNPHYS,D-69117 HEIDELBERG,GERMANY
[5] OSSERVATORIO BRERA,I-20121 MILAN,ITALY
[6] CORNELL UNIV,DEPT ASTRON,ITHACA,NY 14853
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1996年 / 116卷 / 02期
关键词
galaxies; clusters; Coma cluster; interstellar medium; radio lines;
D O I
10.1051/aas:1996108
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present observations of the (CO)-C-12(J=1-0) Line at 2.6 mm of 65 galaxies located in the Coma supercluster region: 33 actually belong to the Coma supercluster while 32 are either foreground or background objects. These data have been obtained using the NRAO 12 m telescope at Kitt Peak (United States), and for four galaxies, using the IRAM 30 m telescope at Pico Veleta (Spain). Out of these 65 galaxies, 54 had never been observed in the CO(1-0) line; 49 have been detected by us, of which 37 are new detections. We give molecular gas masses deduced from the CO Line integrated intensities, and upper limits for the 16 undetected objects, computed with a Galactic conversion factor N(H-2)=2.3 10(20) I(CO) and H-0=75 km/s/Mpc.**
引用
收藏
页码:193 / 202
页数:10
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