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Light-curve and spectral properties of ultra-stripped core-collapse supernovae leading to binary neutron stars
Takashi J. Moriya, Paolo A. Mazzali, Nozomu Tominaga +7
We investigate light-curve and spectral properties of ultra-stripped core-collapse supernovae. Ultra-stripped supernovae are the explosions of heavily stripped massive stars which…
21-year timing of the black-widow pulsar J2051-0827
G. Shaifullah, J. P. W. Verbiest, P. C. C. Freire +23
Timing results for the black-widow pulsar J2051-0827 are presented, using a 21-year dataset from four European Pulsar Timing Array telescopes and the Parkes radio telescope. This d…
Recycled Pulsars: Spins, Masses and Ages
Thomas M. Tauris
Recycled pulsars are mainly characterized by their spin periods, B-fields and masses. All these quantities are affected by previous interactions with a companion star in a binary s…
Models of low-mass helium white dwarfs including gravitational settling, thermal and chemical diffusion, and rotational mixing
Alina Istrate, Pablo Marchant, Thomas M. Tauris +3
A large number of extremely low-mass helium white dwarfs (ELM WDs) have been discovered in recent years. The majority of them are found in close binary systems suggesting they are…
The millisecond pulsar mass distribution: Evidence for bimodality and constraints on the maximum neutron star mass
John Antoniadis, Thomas M. Tauris, Feryal Ozel +3
The mass function of neutron stars (NSs) contains information about the late evolution of massive stars, the supernova explosion mechanism, and the equation-of-state of cold, nucle…
Constraining the ellipticity of strongly magnetized neutron stars powering superluminous supernovae
Takashi J. Moriya, Thomas M. Tauris
Superluminous supernovae (SLSNe) have been suggested to be powered by strongly magnetized, rapidly rotating neutron stars which are often called magnetars. In this process, rotatio…