... 12978 . Daniel E. Welty, University of Chicago . Properties of Diffuse Molecular Gas in the Magellanic Clouds . 12981 . ... the same manner as stars, by gravitational collapse within molecularclouds, but which do not accrete sufficient mass to raise ...
... 455.1001M outbursting protostar of the FU Orionis type in the Cygnus OB7 molecularcloud Movsessian, T. A.; Khanzadyan, T.; Aspin, C.; Magakian, T. Yu.; ...
... easily framed: The very low Jeans mass required to form BDs implies gas densities far in excess of the mean in molecularclouds ... fragmentation' scenario, the high densities arise as fluctuations induced by supersonic turbulence in molecularclouds ...
... are commonly found in the cold molecularclouds that are collapsing in the process ... a small survey of ices in 12 molecularclouds using background stars to obtain ...
... galaxy, and star formation today takes place in dense molecularclouds, while in the early Universe it was hampered by ... and ultimately galaxy formation) hinges on tracing the gravitational collapse of diffuse gas in molecularclouds ...
... Small Magellanic Cloud Ultraviolet Dust Extinction: A Focused Study of Four Sightlines Near a MolecularCloud with Variable 2175 A bumps . 14227 . ...