Stellar studies in the Large Magellanic Cloud. IV - Luminosity function for the bright stars and comparison to the galactic luminosity function

Details Stellar studies in the Large Magellanic Cloud. IV - Luminosity function for the bright stars and comparison to the galactic luminosity function Stellar studies in the Large Magellanic Cloud. IV - Luminosity function for the bright stars and comparison to the galactic luminosity function

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....85..305l&link_type=abstract

Astronomy and Astrophysics, vol. 85, no. 3, May 1980, p. 305-310.

Astronomy and Astrophysics

Astrophysics

22

Astronomical Photography, Galactic Radiation, Magellanic Clouds, Stellar Luminosity, Functions, Interstellar Extinction, Statistical Analysis, Ubv Spectra

Scientific paper

We present a new determination of the luminosity function in photographic magnitudes for the brightest stars in the Large Magellanic Cloud, down to Mpg = -5.5. This luminosity function does not differ significantly in the lower absolute magnitude range from that of the solar neighbourhood nor from those of young galactic clusters and the irregular galaxy IC 1613, indicating similar laws of star formation. However, significant differences in the proportions of very luminous stars (Mpg = -8) appear to exist between the three galaxies.

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