Société Française des Microscopies
By encompassing the magnitude range V < 14, we triple the LMC sample (from 13 to 39). Although both WN (nitrogen-rich) and WC (carbon-rich) stars might ...
Properties of OB star?black hole systems derived from detailed ...time was much higher, and decreased to reach longitudinal homogenization during the high-water phases. ... T.D.; Walker, D.I., 1999. Radial oxygen loss ... In situ observation of new particle formation (NPF) in the tropical ...Calculated TDLDA optical absorption spectrum in the range 2?5 eV for the various protonation states and conformers of the chromopeptide in the ... What can we learn from time-dependent density-functional theory?To obtain an accurate T-X curve, the refractor must be tracked over a sufficiently large range of offsets. In practice, with a targeted ...
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