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KISO H IMAGING OBSERVATIONS OF NEARBY GALAXIES

KISO Htex2html_wrap_inline98 IMAGING OBSERVATIONS OF NEARBY GALAXIES

T. Hasegawa , S. Sakamoto , S. Nishiura , Y. Ohyama , Y. Sofue, PASA, 15 (1), 149
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KISO Htex2html_wrap_inline98 IMAGING OBSERVATIONS OF NEARBY GALAXIES

T. Hasegawa tex2html_wrap_inline100 - S. Sakamoto tex2html_wrap_inline102
S. Nishiura tex2html_wrap_inline104 - Y. Ohyama tex2html_wrap_inline104 - Y. Sofue tex2html_wrap_inline100

tex2html_wrap_inline100 Kiso Observatory, The university of Tokyo
10762-30, Mitake, Kiso, Nagano 397-01, Japan
htakashi@mtk.ioa.s.u-tokyo.ac.jp
tex2html_wrap_inline102 Nobeyama Radio Observatory, National Astronomical Observatory of Japan
Minamimaki, Minamisaku, Nagano 384-13, Japan
seiichi@nro.nao.ac.jp
tex2html_wrap_inline104 Department of Astronomy, Tohoku University
Aoba, Sendai, Miyagi 980-77, Japan

Abstract:

We report Htex2html_wrap_inline98 imaging observations of nearby galaxies with the Kiso Schmidt telescope. For spiral galaxy NGC 628, we found no clear correlation between Htex2html_wrap_inline98 and CO intensities, and we discuss the star formation efficiency of this galaxy. No nuclear Htex2html_wrap_inline98 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 Htex2html_wrap_inline98 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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