Some integrated photometric properties of the Large Magellanic Cloud

Details Some integrated photometric properties of the Large Magellanic Cloud Some integrated photometric properties of the Large Magellanic Cloud

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pasp...90..132h&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 90, Apr.-May 1978, p. 132-138. Research supported by the Carnegie Instit

Astronomy and Astrophysics

Astronomy

12

Astronomical Models, Astronomical Photometry, Magellanic Clouds, Abundance, Brightness, Metals, Planetary Nebulae, Stellar Luminosity

Scientific paper

Central regions of the Large Magellanic Cloud which are free of supergiants were subjected to surface photometry in the UBV and DDO color systems in order to study the properties of the older disk of stars. The surface brightness of the older disk was found to obey, in the central regions examined, the exponential distribution described by Freeman (1970). In spite of obvious differences in structure, the Large Magellanic Cloud and the M33 galaxy appeared to have underlying disks that are analogous.

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