... in a mass range as low as 10-15M. We first recapture the physics of bi-stable winds ... T eff for all FLAMES objects with evolutionary masses above 15M . ... The reason we employ a cut-off mass at 15M is that for the largest subset, i.e ...
... The integrated 1{0 S(1) lobe uxes are 1.4 10 15 W m 2 (North) and 2.7 10 15 W m 2 (South) (Eislo el et al. 1996). ... We employ the integrated 1{0 S(1) K-band uxes of 1.45 10 15 W m 2 (North) and 2.68 10 15 W m 2 (South) tabulated by Eislo el ...
... The Irish Astronomical association AGM will be held at 7.30 p.m. on Wednesday 15 April, in the Bell Lecture Theatre, Physics Building, main campus, QUB. ...
... Gamma 0: m 005, the visual data should be acceptable to \Sigma0: m 08 \Gamma 0: m15 ... data reveal a largeamplitude (\Sigma0: m15) variation; the average V for the data ...
... The observations were performed using the 2k в 4k MIT CCDs (pixel size 15 µm в 15 µm) and a slit width of 1.0 arcsec in order to collect more photons and increase the S/N. We also adopted the 200 kHz/low/1 в 1 readout mode and the GRISM 1200B. Each ...