Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-12-20
Astronomy and Astrophysics
Astrophysics
Latex2e file with 11 postscript figures
Scientific paper
In this paper we study radial oscillations of rotating strange stars in strong magnetic fields in the Density Dependent Quark Mass (DDQM) model. We see that increase of frequency i.e. difference in frequency of rotating and non-rotating stars is more for higher magnetic fields. The change is small for low mass stars but it increases with the mass of the star. This change of frequency is significant for maximum mass whereas it is marginal for a 1.4 solar mass star.
Anand J. D.
Chandrika Devi N.
Gupta Asha
Gupta Vijay K.
Singh Sumeetpal S.
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