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Massive String Cosmology in Bianchi Type III Space-Time with Electromagnetic Field
2010
Communications in Theoretical Physics
O-and B-type stars are often found in binary systems, but the low binary mass-ratio regime is relatively unexplored due to observational difficulties. Binary systems with low mass ratios may have formed through fragmentation of the circumstellar disk rather than molecular cloud core fragmentation. We describe a new technique sensitive to G-and K-type companions to early B stars, a mass ratio of roughly 0.1, using high-resolution, high signal-to-noise spectra. We apply this technique to a sample
doi:10.1088/0253-6102/54/5/32
fatcat:2ttq6dlqtbdx7oikemxoldsizy