H I in barred spiral galaxies. I - NGC 1365

Details H I in barred spiral galaxies. I - NGC 1365 H I in barred spiral galaxies. I - NGC 1365

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...342...29o&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 342, July 1, 1989, p. 29-38. Research supported by the University of Minnes

Astronomy and Astrophysics

Astrophysics

36

Barred Galaxies, Galactic Structure, H Lines, Spiral Galaxies, Emission Spectra, Galactic Bulge, Galactic Rotation, Very Large Array (Vla)

Scientific paper

Neutral hydrogen observations of the barred spiral galaxy NGC 1365 have been made with the Very Large Array with an angular resolution of 24 x 32. The H I is is mostly concentrated in the prominent spiral arms and just outside the bar. No gas is detected in the bar, except that weak H I absorption is seen against the nuclear continuum source at blueshifted velocities, indicating gas outflow. Deviations from circular motion in the gas just outside the bar are consistent with the presence of a strong bar potential. The gas in the spiral arms reveals large streaming motions similar to those seen in galaxies with strong density waves.

Affiliated with

Also associated with

No associations

Rating

H I in barred spiral galaxies. I - NGC 1365 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 H I in barred spiral galaxies. I - NGC 1365, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and H I in barred spiral galaxies. I - NGC 1365 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1703585