The initial mass function for massive stars in the Magellanic Clouds. 1: UBV photometry and color-magnitude diagrams for 14 OB associations

Details The initial mass function for massive stars in the Magellanic Clouds. 1: UBV photometry and color-magnitude diagrams for 14 OB associations The initial mass function for massive stars in the Magellanic Clouds. 1: UBV photometry and color-magnitude diagrams for 14 OB associations

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apjs...91..583h&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 91, no. 2, p. 583-612

Astronomy and Astrophysics

Astrophysics

13

Astronomical Photometry, Color-Magnitude Diagram, Galactic Evolution, Magellanic Clouds, Massive Stars, Open Clusters, Stellar Evolution, Stellar Magnitude, Stellar Mass, Charge Coupled Devices, Chemical Evolution, Error Analysis, Hertzsprung-Russell Diagram, Images, Least Squares Method, Reflecting Telescopes, Stellar Luminosity

Scientific paper

UBV charge coupled device (CCD) photometry has been obtained for 14 OB associations in the Magellanic Clouds using the University of Toronto's 0.6 m telescope and the Carnegie Institution of Washington's 1.0 m reflector, both on Las Campanas, Chile. The data are presented and used to construct color-magnitude diagrams for the purposes of investigating the massive-star content of the associations.

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