CO Observations of Optically Selected Barred Galaxies

Details CO Observations of Optically Selected Barred Galaxies CO Observations of Optically Selected Barred Galaxies

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jkas...31...95l&link_type=abstract

Journal of the Korean Astronomical Society, vol. 31, no. 2, pp. 95-99

Astronomy and Astrophysics

Astronomy

Celestial Mechanics, Stellar Dynamics, Globular Clusters: General

Scientific paper

We report preliminary results of an on-going survey of optically selected barred galaxies with 12CO (J=1-0) line. The entire sample is composed of about 100 bright barred galaxies (B_T <= 13) with small inclination angle. Most of the galaxies are relatively nearby with receding speed less than 10,000 km/sec. In the first observing run, we have observed central parts of 18 galaxies and detected CO emissions from 5 galaxies (NGC 521, 2525, 4262, 4900, and 7479). Most of these galaxies are not observed with CO previously, except for NGC 7479 which has been studied at various wavelength. The peak antenna temperature of detected galaxies ranges from about 30 to 300 mK.

Affiliated with

Also associated with

No associations

Rating

CO Observations of Optically Selected Barred Galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with CO Observations of Optically Selected Barred Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CO Observations of Optically Selected Barred Galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1098138