Stellar and Gas Dynamics in Normal Galaxies Augmentation: Cycle 2 Observations

Details Stellar and Gas Dynamics in Normal Galaxies Augmentation: Cycle 2 Observations Stellar and Gas Dynamics in Normal Galaxies Augmentation: Cycle 2 Observations

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.4062f&link_type=abstract

HST Proposal ID #4062

Physics

Hst Proposal Id #4062

Scientific paper

The FOS will be used with small apertures to map the stellar velocity dispersion and rotation in a grid covering the central 1" of NGC224 (M31). The velocity disperions and rotation curves will be used to model the nuclear dynamics and to measure the nuclear M/L. Line strengths will be used to measure changes in the stellar populations in the central 1". FOS spectra of emission-line clouds within the nuclear region will be used to establish their physical characteristics, ionization mechanisms, and dynamics.

Affiliated with

Also associated with

No associations

Rating

Stellar and Gas Dynamics in Normal Galaxies Augmentation: Cycle 2 Observations 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 Dynamics in Normal Galaxies Augmentation: Cycle 2 Observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar and Gas Dynamics in Normal Galaxies Augmentation: Cycle 2 Observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1207154