Stellar and Gas Kinematics in the Core and Bar Regions of M100

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Galaxies, Star Formation, Kinematics, Spiral Galaxies, Starburst Galaxies And Infrared Excess Galaxies, Kinematics, Dynamics, And Rotation, Proper Motions And Radial Velocities, Space Motions

Scientific paper

Two-dimensional maps of the stellar and gas kinematics of the bar and starbursting circumnuclear region in the barred spiral galaxy M100 are presented. In this progress report, we present maps of the total intensity, mean velocity and velocity dispersion for the stars and the gas. The gas velocity field shows significant kinematic signatures of gas streaming along the inner part of the bar, and across the miniature spiral arms in the nuclear pseudo-ring. The stellar velocity field, presented here for the first time, also shows non-circular motions. The gas velocity dispersion is notably smaller where the star formation occurs in the nuclear zone and HII regions. We outline our further plans with the data set.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Stellar and Gas Kinematics in the Core and Bar Regions of M100 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 Stellar and Gas Kinematics in the Core and Bar Regions of M100, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar and Gas Kinematics in the Core and Bar Regions of M100 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1344972

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.