... merger phase has a constant accretion rate of 104M yr-1 , which makes the merger ... that all models start with fast accretion, i.e. 104M yr-1 , leaving a 0.1 M disc ...
... a total mass of Cyg OB2 of 3 в 104M , similar to that of many of our Galaxy's most ... calculate a total stellar content of 5.7 в 104 stars and a total mass of 2.8 в 104M ...
... stars are significantly less abundant p er unit mass in our Galaxy compared to than that found in globular clusters (eg one p er 4 в 104M for Cen, Olech et al 2005) and dwarf spheroidal galaxies (eg one p er 2.1 в 104M for the Fornax dSph, Poretti et al ...
... The post-merger evolution was modelled by considering fast accretion at 104M yr-1 (representing the formation of a hot corona), followed by slow accretion at 10-5 M yr-1 (representing accretion from a Keplerian disc). ...
... Recent claims for the existence of very massive stars (VMS) of up to 300 M at the centre of young clusters like R136 (Crowther et al. 2010) seem to link the formation of such objects to environments in the centres of massive clusters with 104 - 105 M ...
... 104] V. M. Bogod, G. B. Gelfreikh, Measurements of the magnetic field and the gradient of temperature in the solar atmosphere above a flocculus using radio observations, Sol. ...
... 40 survey fields spanning three nights covering 11 square degrees near opposition, using the Wide Field Camera on the 2.5 m Isaac Newton Telescope (INT), resulting in 104 discovered main belt asteroids (MBAs) and another 626 unknown one-night objects ...