Model atmospheres and X-ray spectra of iron-rich bursting neutron stars. II. Iron rich Comptonized Spectra

Kavli Affiliate: P. C. Joss| First 5 Authors: A. Majczyna, A. Majczyna, , , | Summary:This paper presents the set of plane-parallel model atmosphere equations for a very hot neutron star (X-ray burst source). The model equations assume both hydrostatic and radiative equilibrium, and the equation of state of an ideal gas in local thermodynamic […]


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The BaBar Event Building and Level-3 Trigger Farm Upgrade

Kavli Affiliate: Steffen Luitz| First 5 Authors: S. Luitz, S. Luitz, , , | Summary:The BaBar experiment is the particle detector at the PEP-II B-factory facility at the Stanford Linear Accelerator Center. During the summer shutdown 2002 the BaBar Event Building and Level-3 trigger farm were upgraded from 60 Sun Ultra-5 machines and 100MBit/s Ethernet […]


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Ratio of color and effective temperatures in X-ray burst spectra

Kavli Affiliate: P. C. Joss| First 5 Authors: A. Majczyna, A. Majczyna, , , | Summary:We present model atmospheres and theoretical spectra for X-ray bursters. Our models include the effects of Compton scattering on free electrons. The atmospheres have compositions that are mixtures of hydrogen, helium, and iron. For our models the ratio of color […]


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HE 0435-1223: a wide separation quadruple QSO and gravitational lens

Kavli Affiliate: Edmund Bertschinger| First 5 Authors: Lutz Wisotzki, Lutz Wisotzki, , , | Summary:We report the discovery of a new gravitationally lensed QSO, at a redshift z = 1.689, with four QSO components in a cross-shaped arrangement around a bright galaxy. The maximum separation between images is 2.6 arcsec, enabling a reliable decomposition of […]


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Special McKay correspondence

Kavli Affiliate: Yukari Ito| First 5 Authors: Yukari Ito, Yukari Ito, , , | Summary:There are many generalizations of the McKay correspondence for higher dimensional Gorenstein quotient singularities and there are some applications to compute the topological invariants today. But some of the invariants are completely different from the classical invariants, in particular for non-Gorenstein […]


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