STIS Far UV Images and Broadband Colors of Galaxies at z=0.1

Details STIS Far UV Images and Broadband Colors of Galaxies at z=0.1 STIS Far UV Images and Broadband Colors of Galaxies at z=0.1

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.0815m&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #08.15; Bulletin of the American Astronomical Society, Vol. 30, p.1260

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As part of a project to investigate the morphological properties of normal galaxies in the far ultraviolet (FUV) we have obtained STIS FUV images of 7 fields which include 13 detectable galaxies. The galaxies are all in groups associated with a bright (3C) radio galaxy at redshifts between z=0.1 and z=0.2. Follow-up ground-based images in U, B, V, R and I have been obtained using the 2-m telescope at KPNO. In addition to the STIS FUV images STIS broadband ( ~ 3000-10000 Angstroms) CCD images were obtained. These high resolution images have been used to classify the morphological type of each galaxy. We present the FUV, U, B, V, R, I spectral energy distribution as a function of morphological type and examine where within each galaxy the FUV light originates.

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