NDLI: Simulating a White Dwarf-dominated Galactic Halo

Content Provider	Semantic Scholar
Author	Brook, Chris B. Kawata, Daisuke Gibson, Brad K.
Abstract	Observational evidence has suggested the possibility of a Galactic halo which is dominated by white dwarfs (WDs). While debate continues concerning the interpretation of this evidence, it is clear that an initial mass function (IMF) biased heavily toward WD precursors (1
File Format	PDF HTM / HTML
Alternate Webpage(s)	http://cds.cern.ch/record/614905/files/0305014.pdf
Language	English
Access Restriction	Open
Subject Keyword	Bethe–Salpeter equation DWARF Dark Matter Emoticon Filamentous fungus Galaxy Greater Than Halo nevus Halo: Combat Evolved Anniversary Leukocytes Mass fraction Medical Subject Headings Numerical analysis Offset binary Oxygen Population Parameter Semiconductor industry Simulation Smoothed-particle hydrodynamics Smoothing Stars, Celestial
Content Type	Text
Resource Type	Article

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