A comparison of star formation characteristics in different types of irregular galaxies

Details A comparison of star formation characteristics in different types of irregular galaxies A comparison of star formation characteristics in different types of irregular galaxies

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nasa.reptq....l&link_type=abstract

Final Technical Report National Aeronautics and Space Administration. Ames Research Center, Moffett Field, CA.

Physics

Cosmology, Energy Distribution, Irregular Galaxies, Morphology, Stellar Evolution, Galactic Evolution, Iue, Line Spectra, Stellar Physics, Ultraviolet Spectra

Scientific paper

Two regions of recent star formation in blue irregular galaxies were
observed with the IUE in the short wavelength, low dispersion mode. The
spectra indicates that the massive star content is similar in these
regions and is best fit by massive stars formed in a burst and now are
approximately 2.5 to 3.0 million years old.

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