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X-ray, UV, and optical observations of the accretion disk and boundary layer in the symbiotic star RT Crucis
(EDP Sciences, 2018-05)
Compared to mass transfer in cataclysmic variables, the nature of accretion in symbiotic binaries in which red giants transfer material to white dwarfs (WDs) has been difficult to uncover. The accretion flows in a symbiotic ...
Magnetic field decay in black widow pulsars
(Wiley Blackwell Publishing, Inc, 2018-04)
We study in this work the evolution of the magnetic field in 'redback-black widow' pulsars. Evolutionary calculations of these 'spider' systems suggest that first the accretion operates in the redback stage, and later the ...
Forward-backward approximation of evolution equations in finite and infinite horizon
(Amer Inst Mathematical Sciences-Aims, 2021)
This research is concerned with evolution equations and their forward-backward discretizations.
Our rst contribution is an estimation for the distance between iterates of sequences
generated by forward-backward schemes, ...
Some limit results for integrands and Hamiltonians with applicaiton to viscosity
(2005)
The present work is essentially a continuation of [10], [6], [7] dealing withControl problems where the dynamics are driven by ordinary differentialequations (ODE) [9] and evolution inclusions (EI) governed by nonconvexsweeping ...
Internal heating of old neutron stars: contrasting different mechanisms
(2010)
Context: The standard cooling models of neutron stars predict temperatures T<104 K for ages t>107 yr. However, the likely thermal emission detected from the millisecond pulsar J0437-4715, of spin-down age ts∼7×109 yr, ...