Generation of massive stellar black holes by rapid gas accretion in ...

The mass function (MF) measured at the half-mass radius, and as such representative of the cluster's global properties, is surprisingly flat. Over the range.







The Impact of Dust on the Sizes of Galaxies in the Epoch of ...
At a time t = tD + ?, half of the initial gas mass is driven out. In that respect, ? differs from the gas expulsion time scale adopted in Geyer.
The black hole retention fraction in star clusters - Sirrah
We present the first study of the dynamical evolution of an isolated star cluster that combines a significant population of primordial binaries with the ...
Development and quality evaluation of aloe vera gel ice cube
It is shown that the requirement of 7 ns is well achieved allowing for plenty of leeway for other uncertainties, which may arise after the DOMs are deployed.



Autres Cours:

Development of a half-meter scale Traveling-Wave (TW) SRF cavity