The Nature of the Central UV Source in M31

Details The Nature of the Central UV Source in M31 The Nature of the Central UV Source in M31

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.6300f&link_type=abstract

HST Proposal ID #6300

Physics

Hst Proposal Id #6300 Agn

Scientific paper

The FOS will be used with small apertures to map the stellarvelocity
dispersion and rotation in a grid covering the central 0.5"of NGC224
(M31). The velocity disperions and rotation curves will beused to model
the nuclear dynamics and to measure the nuclear M/L.

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