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- W2087339766 abstract "view Abstract Citations (26) References (24) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Studies of the Large Magellanic Cloud.VI. Properties of 1057 Field Stars. Hodge, Paul W. Abstract Color-magnitude diagrams of field stars are presented for two relatively open areas of the Large Magellanic Cloud. In the larger area, 933 stars have been measured in a sampling which is complete to V = 17 and extends to V = 18. The color-magnitude diagram for this region shows a strong main sequence, accounting for about half the stars, and concentrations of giants and supergiants at B - V = +0.8 and +2.0. A strongly populated giant region is made up primarily of stars evolved from the main sequence fainter than the limit of the photometry, probably globular cluster-like stars. The color- magnitude array for the second region, which is the farther from the center of the Cloud, shows a weakly populated main sequence, relative to the number of giants. Luminosity functions for the two regions do not agree; the more central area has an overabundance of bright stars with respect to the van Rhijn function, while the second area's luminosity function agrees very closely with that of the solar neighborhood. A stellar association resembles in sixe, age, and shape the young star associations in our Galaxy. Publication: The Astrophysical Journal Supplement Series Pub Date: June 1961 DOI: 10.1086/190065 Bibcode: 1961ApJS....6..235H full text sources ADS | data products SIMBAD (13) Related Materials (9) Part 1: 1960ApJ...131..351H Part 2: 1960ApJ...132..341H Part 3: 1960ApJ...132..346H Part 4: 1960ApJ...132..351H Part 5: 1961ApJ...133..413H Part 7: 1961ApJ...134..226H Part 8: 1963ApJ...137.1033H Part 9: 1963ApJ...138..366H Part 10: 1969ApJS...17..467H" @default.
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- W2087339766 date "1961-06-01" @default.
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- W2087339766 title "Studies of the Large Magellanic Cloud.VI. Properties of 1057 Field Stars." @default.
- W2087339766 doi "https://doi.org/10.1086/190065" @default.
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