... 9. Multiple stellar populations in massive LMC star clusters . ... 3. Core evolution of rich stellar clusters in the LMC . ... p. 423 . 2. Dynamical evolution of LMC star clusters . ...
... to 0.6 M Sun , except for a few Peimbert Type I nebulae (e.g., NGC 6302 with 0.8 M Sun , or a handful of objects in the LMC ... resolution of a little better than 0.1", which corresponds to a linear resolution of ~ 0.02 pc at the distance of the LMC ...
... evolution of Planetary Nebulae (PN) in the Large Magellanic Cloud (LMC) are given ... we derive, for the first time, the chemical history of the LMC using PN as tracers ...
... SN 1987A. In measuring their Hubble Constant of 72 km/s/Mpc, the Key Project assumed that the LMC was located 50kpc from Earth ... What Hubble constant would they have gotten if they had used your distance to the LMC?. ...
... clusters in the Large Magellanic Cloud (LMC), produced a very interesting and ... clusters, the dSph satellites and the LMC, the initiation of star formation among ... is tearing apart its companion galaxies (the LMC and SMC) with gravitational tides ...
... MACHO Observations of LMC Red Giants: definite pulsators and possible binary stars . ... has monitored stars in the Large Magellanic Cloud (LMC) almost daily for more than 6 ...
... This result was recently published, and is especially significant in the light of recent suggestions that the LMC lenses may not in fact be in the halo, but rather are in an intervening strand of material tidally stripped from the LMC. ...