Stellar and Gas Dynamics in Normal Galaxies Augmentation - Cycle 4 Carryover

Details Stellar and Gas Dynamics in Normal Galaxies Augmentation - Cycle 4 Carryover Stellar and Gas Dynamics in Normal Galaxies Augmentation - Cycle 4 Carryover

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5744f&link_type=abstract

HST Proposal ID #5744

Physics

Hst Proposal Id #5744 Galaxies &Amp, Clusters

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.

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