An IUE search for star formation in ellipticals with gaseous disks

Details An IUE search for star formation in ellipticals with gaseous disks An IUE search for star formation in ellipticals with gaseous disks

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...403..577b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 403, no. 2, p. 577-580.

Astronomy and Astrophysics

Astrophysics

4

Elliptical Galaxies, Galactic Structure, Interstellar Gas, Iue, Star Formation, Absorption Spectra, Interstellar Extinction, Red Shift, Spectral Energy Distribution

Scientific paper

The UV spectral energy distribution presently derived from IUE observations for NGC 5077 is presently compared with those of the bulges of two galaxies, M31 and NGC 3115, which exhibit a similar Mg2 absorption-liner strengths and are known to lack gaseous disks. The lack of significant UV spectrum differences imply that there is no star formation activity more recent than 3 million years old in NGC 5077.

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