Central Dark and Baryonic Mass Distribution in the Isolated Barred Galaxy NGC 3367

Details Central Dark and Baryonic Mass Distribution in the Isolated Barred Galaxy NGC 3367 Central Dark and Baryonic Mass Distribution in the Isolated Barred Galaxy NGC 3367

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..34..117c&link_type=abstract

IV Reunión sobre Astronomía Dinámica en Latino América (Eds. C. Allen, A. Ruelas, & R. Teixeira) Revista Mexicana de Astronomía

Astronomy and Astrophysics

Astronomy

Dark Matter, Galaxies: Bulges, Galaxies: Individual (Ngc 3367)

Scientific paper

We have initiated a project that aims to revise the robustness of the suggestions of the dearth of dark matter in the central regions of barred galaxies through a detailed study of the galaxy NGC 3367. The internal kinematics of this galaxy has been measured in ionized and molecular gas and in the stellar component, making it a good benchmark for dynamical studies because it allows us to analyze the biases associated with each tracer. >From our observations we will directly measure the bar pattern speed, a property that has been considered as a free parameter in all previous studies.

Affiliated with

Also associated with

No associations

Rating

Central Dark and Baryonic Mass Distribution in the Isolated Barred Galaxy NGC 3367 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 Central Dark and Baryonic Mass Distribution in the Isolated Barred Galaxy NGC 3367, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Central Dark and Baryonic Mass Distribution in the Isolated Barred Galaxy NGC 3367 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-795680