STIS Key Project: The nuclear region of NGC 4151 Observations

Details STIS Key Project: The nuclear region of NGC 4151 Observations STIS Key Project: The nuclear region of NGC 4151 Observations

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000hst..prop.8473h&link_type=abstract

HST Proposal ID #8473

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Hst Proposal Id #8473

Scientific paper

The Seyfert 1 galaxy NGC 4151 will be studied in several ways. 1} Low-resolution spectra over the entire UV and visible range will be obtained through a slit at several different orientations to model the physical conditions in the emission-line regions; 2} slitless and long-slit spectra of strong emission lines at moderate resolution and narrow-band WFPC2 images will be used to map the dynamics of the regions; 3}echelle spectra over the entire UV bandpass will be used to study the intrinsic absorption in the nucleus; and 4} parallel imaging will be performed of the outer galaxy and other galaxies or QSOs.

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