40 Years of Pulsars : Millisecond Pulsars, Magnetars and More

By Cees G. Bassa, Zhongxiang Wang, A. Cumming, Victoria Kaspi. 2008

398 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/c3213fd6f0b3e9d25d1badb7afbfa4fbe9fe90db

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Citations in the corpus

Protoneutron star evolution and the neutrino-driven wind in general relativistic neutrino radiation hydrodynamics simulations (2009, background): “Present axially symmetric core collapse models of massive Fe-core progenitor stars (even non-rotating) predict bipolar explosions (see Janka et al. (2008)).”
Further searches for Rotating Radio Transients in the Parkes Multi-beam Pulsar Survey (2009, background): “In addition to pulsars and c© 0000 RAS, MNRAS 000, 000–000 RRATs there are the INSs, magnetars, neutron stars in accreting binary systems and the Central Compact Objects (of which some are thought to be neutron stars, e.g. see de Luca (2008)).”
Gravitational waves from resolvable massive black hole binary systems and observations with Pulsar Timing Arrays (2008, background): “The complete Parkes PTA (Manchester 2008), the European Pulsar Timing Array (Janssen et al. 2008), and NanoGrav 1 are expected to improve considerably on the capabilities of these surveys and the planned Square Kilometer Array (SKA; www.skatelescope.org) will produce a major leap in sensitivity.”
THE LOCATIONS OF SHORT GAMMA-RAY BURSTS AS EVIDENCE FOR COMPACT OBJECT BINARY PROGENITORS (2013, background): “2 s), several theoretical progenitor systems have been proposed, including NS-NS/NS-BH mergers (Eichler et al. 1989; Narayan et al. 1992), accretioninduced-collapse of a WD or NS (Qin et al. 1998; Levan et al. 2006; Metzger et al. 2008) and magnetar flares (Levan et al. 2006; Chapman et al. 2008).”