M31 vs. M33: Different modes of star formation

Details M31 vs. M33: Different modes of star formation M31 vs. M33: Different modes of star formation

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..393..475h&link_type=abstract

The seventh astrophysical conference: Star formation, near and far. AIP Conference Proceedings, Volume 393, pp. 475-477 (1997).

Astronomy and Astrophysics

Astrophysics

Hii Regions, Emission And Reflection Nebulae, Origin, Formation, Evolution, Age, And Star Formation, Magnitudes And Colors, Luminosities, Star Formation

Scientific paper

Among the various differences in star-formation modes between various
types of galaxies, the differences in HII region luminosity functions
are conspicuous. A comparison of those of M31 and M33, using new data,
illustrates these differences, which are best understood in terms of
different stellar clustering mass functions for the galaxies.

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