output
19932026
Showing 2013 · astro-ph.HEShow all

15 papers · 2 filters

astro-ph.HE2013★ 225 cited

A state change in the missing link binary pulsar system PSR J1023+0038

B. W. Stappers, A. M. Archibald, J. W. T. Hessels +9

We present radio, X-ray, and gamma-ray observations which reveal that the binary millisecond pulsar / low-mass X-ray binary transition system PSR J1023+0038 has undergone a transfo…

astro-ph.HE2013★ 170 cited

A New Accretion Disk Around the Missing Link Binary System PSR J1023+0038

A. Patruno, A. M. Archibald, J. W. T. Hessels +7

PSR J1023+0038 is an exceptional system for understanding how slowly rotating neutron stars are spun up to millisecond rotational periods through accretion from a companion star. O…

astro-ph.HE2013★ 96 cited

The neutron star transient and millisecond pulsar in M28: from sub-luminous accretion to rotation-powered quiescence

Manuel Linares, Arash Bahramian, Craig Heinke +6

The X-ray transient IGR J18245-2452 in the globular cluster M28 contains the first neutron star (NS) seen to switch between rotation-powered and accretion-powered pulsations. We an…

astro-ph.HE2013★ 15 cited

Double-peaked thermonuclear bursts at the soft-hard state transition in the Rapid Burster

T. Bagnoli, J. J. M. in 't Zand, A. Patruno +1

Long suspected to be due to unstable accretion events, the type II bursts exhibited by the Rapid Burster (RB, or MXB 1730-335) still lack an exhaustive explanation. Apart from type…

astro-ph.HE2013★ 38 cited

Broadband monitoring tracing the evolution of the jet and disk in the black hole candidate X-ray binary MAXI J1659-152

A. J. van der Horst, P. A. Curran, J. C. A. Miller-Jones +31

MAXI J1659-152 was discovered on 2010 September 25 as a new X-ray transient, initially identified as a gamma-ray burst, but was later shown to be a new X-ray binary with a black ho…

astro-ph.HE2013★ 17 cited

Constraining white dwarf viscosity through tidal heating in detached binary systems

Simone Dall'Osso, Elena Maria Rossi

Although the internal structure of white dwarfs is considered to be generally well understood, the source and entity of viscosity is still very uncertain. We propose here to study…