Have we observed the skin vibration of realistic strange stars (ReSS) ?
arXiv:astro-ph/0211612 · doi:10.1142/S0217732303009782
Abstract
Skin vibration of ReSS and consequent resonance absorption can account for the absorption lines in the spectrum of X-ray emission from many compact stellar objects and in particular, the stars J12105226 and RXJ18563754. Observations of the X-ray spectrum of these stars is difficult to explain, if they are neutron stars.
7 pages, 2 figures
References in corpus (12)
- Gravitationally redshifted absorption lines in the X-ray burst spectra of a neutron star
- Is SAX J1808.4-3658 a Strange Star ?
- Towards a Mass and Radius Determination of the Nearby Isolated Neutron Star RX J185635-3754
- Conversion of neutron stars to strange stars as the central engine of gamma-ray bursts
- Bare Quark Matter Surfaces of Strange Stars and Emission
- Quark-Nova
- On the nature of the compact star in 4U 1728-34
- Thermal emission from bare quark matter surfaces of hot strange stars
- Small strange stars and marginally stable orbit in Newtonian theory
- Superbursts and long bursts as surface phenomenon of compact objects
- Rapidly rotating strange stars for a new equation of state of strange quark matter
- Stability of strange stars (SS) derived from a realistic equation of state
Cited by in corpus (10)
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- Possible evidence of surface vibration of strange stars from stellar observations
- Evidence for strange stars from joint observation of harmonic absorption bands and of redshift
- Newtonian and general relativistic contribution of gravity to surface tension of strange stars
- Decoupling of pion coupling f_π from quarks at high density in three models, and its possible observational consequences
- Addendum to ``Decoupling of pion coupling from quarks at high density in three models, and its possible observational consequences"
- Chromo-thermal oscillations and collapse of strange stars to black holes : Astrophysical Implications
- Bound for entropy and viscosity ratio for strange quark matter
- Strange Star Equation of State With a Modified Richardson Potential