Optical Spectroscopy of Massive Binary Stars
This is a spectroscopic and photometric study of suspected close binary systems among the massive stars. The stars studied here include stars with temperatures ranging from 45,000 Kelvin (K) to 15,000 K, corresponding to spectral types ranging from O3 V to B5 III, masses between 47 Solar Masses and...
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| Format: | Others |
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Digital Archive @ GSU
2011
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| Online Access: | http://digitalarchive.gsu.edu/phy_astr_diss/49 http://digitalarchive.gsu.edu/cgi/viewcontent.cgi?article=1048&context=phy_astr_diss |