Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998pasj...50..317s&link_type=abstract
Publications of the Astronomical Society of Japan, v.50, p.317-323.
Astronomy and Astrophysics
Astronomy
10
Galaxies: Active, Galaxies: Evolution, Galaxies: Individual (Ngc 4736), Stars: Formation
Scientific paper
We present (12) CO (J=1--0) observations of the poststarburst nucleus of NGC 4736. Although star in the nuclear region is currently inactive, there is a substantial amount of molecular gas, ~ 10(7 MO ) , in the central ~ 300 pc region. Comparing the observed molecular-gas surface density with the threshold gas density for star formation proposed by Kennicutt (1989, AAA 50.157.264), we find that the nuclear gas disk is stable for gravitational instability. We discuss possible scenarios for the nuclear starburst evolution of NGC 4736 in terms of either bar-driven instability fueling or minor-merger driven fueling (or triggering).
Ishizuki Sumio
Murayama Takashi
Ohyama Youichi
Shioya Yasuhiro
Taniguchi Yoshiaki
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