Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.250..679b&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 250, June 15, 1991, p. 679-682. Research supported by C
Astronomy and Astrophysics
Astrophysics
11
Nuclear Astrophysics, Radio Stars, Stellar Composition, Stellar Oscillations, Pulsars, Radial Distribution, Stellar Interiors
Scientific paper
A study presented for neutron star radial oscillations by Lindblom and Detweiler (1983), where a wide set of equations of state were employed to extract the oscillatory features of those stars, is drawn on to examine a similar analysis corresponding to homogeneous strange star models. The general features and numerical results for radial pulsations are addressed. The particular form of the equation of state is shown to allow some simple and general scaling relations which may prove very useful for the search for the stars. The physical conditions for excitation and damping of radial modes, as well as their possible observation signatures, are discussed. It is found that all potentially important oscillation modes can be used to distinguish strange from neutron stars.
Benvenuto Omar G.
Horvath Jorge Ernesto
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