IMAGING OBSERVATIONS OF NEARBY GALAXIES T. Hasegawa , S. Sakamoto , S. Nishiura , Y. Ohyama , Y. Sofue, PASA, 15 (1), 149
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Next Section: INTRODUCTION
KISO H
IMAGING OBSERVATIONS OF NEARBY GALAXIES
T. Hasegawa 
- S. Sakamoto 
S. Nishiura 
- Y. Ohyama - Y. Sofue
Kiso Observatory, The university of Tokyo
10762-30, Mitake, Kiso, Nagano 397-01, Japan
htakashi@mtk.ioa.s.u-tokyo.ac.jp Nobeyama Radio Observatory, National Astronomical Observatory of Japan
Minamimaki, Minamisaku, Nagano 384-13, Japan
seiichi@nro.nao.ac.jp Department of Astronomy, Tohoku University
Aoba, Sendai, Miyagi 980-77, Japan
Abstract:
We report H imaging observations of nearby galaxies with the Kiso Schmidt telescope. For spiral galaxy NGC 628, we found no clear correlation between H and CO intensities, and we discuss the star formation efficiency of this galaxy. No nuclear H emission in this galaxy was detected. This is consistent with spectroscopic observations which indicate that the nuclear region is in the post starburst phase. We also describe the H image of Hickson's compact group 92 in which diffuse emission is detected extending within the group system.
Keywords: galaxies: ISM -- infrared: galaxies -- radio lines: galaxies
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