Nuclei of Nearly Normal Galaxies (WF/PC-14) - Repeat for HOPR# 0008

Details Nuclei of Nearly Normal Galaxies (WF/PC-14) - Repeat for HOPR# 0008 Nuclei of Nearly Normal Galaxies (WF/PC-14) - Repeat for HOPR# 0008

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3410w&link_type=abstract

HST Proposal ID #3410

Other

Hst Proposal Id #3410 Galaxies &Amp, Clusters

Scientific paper

Direct images of the nuclei of nearby galaxies taken with the Planetary Camera will be used to measure the space density profile of luminous material and the nuclear color gradients in these objects. Galaxies will be imaged with the F555W and F785LP filters. Serveral objects known to contain ionized gas will also be imaged in narrow-band filters to obtain the gas distribution. In M31 a special series of ultra-violet exposures will be taken to study the hot stellar population. The sample of objects contains several normal ellipticals covering a broad range in nuclear surface brightness and concentration class, several nearby galaxies covering a range of Hubble types, and a few Seyfert and otherwise slightly abnormal nuclei.The images taken will also be searched for bright stars, inner globular clusters, and absorbing interstellar dust.

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