Uniformity of the WC stars in the Large Magellanic Cloud

Results on the uniformity of the WC stars in the LMC are presented. It is shown to be a tenable hypothesis that (b-v)sub 0 is the same for all observed stars, thus enabling estimates of absorption in the 30 Dor region where local irregularities are large. The flux in the C IV lambda 5808 line is 3 x...

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Veröffentlicht in:	The Astrophysical journal 1990, Vol.348 (2), p.471-484
Hauptverfasser:	SMITH, L. F, SHARA, M. M, MOFFAT, A. F. J
Format:	Artikel
Sprache:	eng
Schlagworte:	640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources 640105 - Astrophysics & Cosmology- Galaxies Astronomy CARBON STARS CHARGE-COUPLED DEVICES CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COLOR DISTANCE DISTRIBUTION Earth, ocean, space EMISSION SPECTRA Emission-line stars (of, be, luminous blue variables, wolf-rayet, etc.) Exact sciences and technology GALAXIES INTERSTELLAR SPACE LINE WIDTHS MAGELLANIC CLOUDS MAIN SEQUENCE STARS MEASURING METHODS OPTICAL PROPERTIES ORGANOLEPTIC PROPERTIES PHYSICAL PROPERTIES SEMICONDUCTOR DEVICES SPACE SPATIAL DISTRIBUTION SPECTRA SPECTROPHOTOMETRY STARS Variable and peculiar stars (including novae) WOLF-RAYET STARS
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