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Multi-colour optical light curves of the companion star to the millisecond pulsar PSR J2051-0827
V. S. Dhillon, M. R. Kennedy, R. P. Breton +16
We present simultaneous, multi-colour optical light curves of the companion star to the black-widow pulsar PSR J2051-0827, obtained approximately 10 years apart using ULTRACAM and…
An irradiated brown-dwarf companion to an accreting white dwarf
Juan V. Hernández Santisteban, Christian Knigge, Stuart P. Littlefair +7
Brown dwarfs and giant planets orbiting close to a host star are subjected to significant irradiation that can modify the properties of their atmospheres. In order to test the atmo…
A LOFAR census of non-recycled pulsars: average profiles, dispersion measures, flux densities, and spectra
A. Bilous, V. Kondratiev, M. Kramer +24
We present first results from a LOFAR census of non-recycled pulsars. The census includes almost all such pulsars known (194 sources) at declinations and Galac…
The long-term evolution of the X-ray pulsar XTE J1814-338: a receding jet contribution to the quiescent optical emission?
Maria Cristina Baglio, Paolo D'Avanzo, Teo Munoz-Darias +2
We present a study of the quiescent optical counterpart of the Accreting Millisecond X-ray Pulsar XTE J1814-338, carrying out multiband (BVR) orbital phase-resolved photometry usin…
The double pulsar: evidence for neutron star formation without an iron core-collapse supernova
R. D. Ferdman, I. H. Stairs, M. Kramer +8
The double pulsar system PSR J0737-3039A/B is a double neutron star binary, with a 2.4-hour orbital period, which has allowed measurement of relativistic orbital perturbations to h…
KOI 1224, a Fourth Bloated Hot White Dwarf Companion Found With Kepler
Rene P. Breton, Saul A. Rappaport, Marten H. van Kerkwijk +1
We present an analysis and interpretation of the Kepler binary system KOI 1224. This is the fourth binary found with Kepler that consists of a thermally bloated, hot white dwarf in…