Chemical Evolution Model of M33

Details Chemical Evolution Model of M33 Chemical Evolution Model of M33

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..129r&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a chemical evolution model (CEM) of M33 and we find that M33,
which is smaller than both M31 and MW, shows a lower gas infall rate,
SFR efficiency, and IMF M_{up}. Therefore the CEMs for large spiral
galaxies (Carigi et al. 2005; Meneses-Goytia et al. 2011) can be scaled
to a smaller galaxy.

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