Star Counts in Fields Surrounding the Large Magellanic Cloud

Details Star Counts in Fields Surrounding the Large Magellanic Cloud Star Counts in Fields Surrounding the Large Magellanic Cloud

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108...97b&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Physics

2

Scientific paper

Star counts in a number of fields near the Large Magellanic Cloud have
shown a maximum extension of about 10° for the faint stars. The
luminosity function in the outer regions of the LMC is consistent with
an intermediate age population.

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