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2006MNRAS.371.1351B - Mon. Not. R. Astron. Soc., 371, 1351-1358 (2006/September-3)
White dwarf stars as strange quark matter detectors - III.
BENVENUTO O.G.
Abstract (from CDS):
The characteristics of the spectrum of oscillations of strange dwarf stars are very different from the ones corresponding to normal white dwarfs and should be, in principle, observable. Consequently, the stars usually considered as white dwarfs may indeed provide an interesting and affordable way to detect SQM in an astrophysical environment.
Abstract Copyright: 2006 The Author. Journal compilation © 2006 RAS
Journal keyword(s): dense matter - stars: oscillations - white dwarfs
Simbad objects: 1
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