Results 281 to 290 of about 261,811 (317)
V3101 Cyg: A Cataclysmic Variable Born with a Brown Dwarf Donor
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Astrophysics and Space Science, 1971
Neutron star models are calculated using an equation of state discussed in an earlier paper. A maximum mass for a neutron star of 1.74 solar masses is found. The central density of thie star is 3.3×1015 g/cm3. The lightest stars have masses of 0.02 (resp. 0.03) solar masses with central densities 2.2×1014 g/cm3 (resp. 1.9×1014).
Gerhard B�rner, Katsuhiko Sato
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Neutron star models are calculated using an equation of state discussed in an earlier paper. A maximum mass for a neutron star of 1.74 solar masses is found. The central density of thie star is 3.3×1015 g/cm3. The lightest stars have masses of 0.02 (resp. 0.03) solar masses with central densities 2.2×1014 g/cm3 (resp. 1.9×1014).
Gerhard B�rner, Katsuhiko Sato
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Stability of Quark Star Models
Communications in Theoretical Physics, 2016Summary: In this paper, we investigate the stability of quark stars with four different types of inner matter configurations; isotropic, charged isotropic, anisotropic and charged anisotropic by using the concept of cracking. For this purpose, we have applied local density perturbations technique to the hydrostatic equilibrium equation as well as on ...
Azam, M., Mardan, S. A., Rehman, M. A.
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Star-Star Relation for the Potts Model
International Journal of Modern Physics B, 1997A star-star transformation is introduced for the Potts model as a generalization of the Onsager star-triangle relation. By considering a special limit of the star-star relation, we deduce a dual transformation relation for the Potts model on the 3-12 lattice.
C. King, F. Y. Wu
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International Astronomical Union Colloquium, 1976
PhenomenologyThe outstanding observational facts that impress the theorist studying the magnetic Ap stars are as follows:1) The very strong, large-scale magnetic fields, inferred from the integrated Zeeman effect. Typical polar fields are 103- 104gauss, the strongest known being =3.5 x 104gauss.2) The variability of the fields, spectra and luminosities,
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PhenomenologyThe outstanding observational facts that impress the theorist studying the magnetic Ap stars are as follows:1) The very strong, large-scale magnetic fields, inferred from the integrated Zeeman effect. Typical polar fields are 103- 104gauss, the strongest known being =3.5 x 104gauss.2) The variability of the fields, spectra and luminosities,
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HYDRODYNAMICAL MODELS OF GASEOUS STARS
Reviews in Mathematical Physics, 1996We revisit the main results concerning the local and global existence and the stability of solutions for some simplified models of self-gravitating stars used in astrophysical hydrodynamics, with an emphasis on the spherical situation.
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Relativistic Model for Radiating Star
Astrophysics and Space Science, 2006zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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Antibody–drug conjugates: Smart chemotherapy delivery across tumor histologies
Ca-A Cancer Journal for Clinicians, 2022Paolo Tarantino +2 more
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An overview of real‐world data sources for oncology and considerations for research
Ca-A Cancer Journal for Clinicians, 2022Lynne Penberthy +2 more
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