activity
20062017
most citedEpisodic Accretion on to Strongly Magnetic Stars

209 citations · 1.2k across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.SR2017★ 47 cited

Magnetically gated accretion in an accreting 'non-magnetic' white dwarf

S. Scaringi, T. J. Macarone, C. D'Angelo +2

White dwarfs are often found in binary systems with orbital periods ranging from tens of minutes to hours in which they can accrete gas from their companion stars. In about 15% of…

astro-ph.HE2017★ 67 cited

Simultaneous Chandra and VLA Observations of the Transitional Millisecond Pulsar PSR J1023+0038: Anti-correlated X-ray and Radio Variability

Slavko Bogdanov, Adam T. Deller, James C. A. Miller-Jones +6

We present coordinated Chandra X-ray Observatory and Karl G. Jansky Very Large Array observations of the transitional millisecond pulsar PSR J1023+0038 in its low-luminosity accret…

astro-ph.HE2017★ 69 cited

Disk-jet coupling in low-luminosity accreting neutron stars

V. Tudor, J. C. A. Miller-Jones, A. Patruno +12

In outburst, neutron star X-ray binaries produce less powerful jets than black holes at a given X-ray luminosity. This has made them more difficult to study as they fade towards qu…

astro-ph.HE2017★ 2 cited

Chandra spectroscopy of Rapid Burster type-I X-ray bursts

J. J. M. in 't Zand, T. Bagnoli, C. D'Angelo +5

We observed the Rapid Burster with Chandra when it was in the 'banana' state that usually precedes the type-II X-ray bursting 'island' state for which the source is particularly kn…

astro-ph.HE2017★ 12 cited

The X-ray Pulsar 2A 1822-371 as a Super Eddington source

A. Bak Nielsen, A. Patruno, C. D'Angelo

The low mass X-ray binary 2A 1822-371 is an eclipsing system with an accretion disc corona and with an orbital period of 5.57 hr. The primary is an 0.59 s X-ray pulsar with a propo…

astro-ph.HE2016★ 80 cited

Timing Observations of PSR J1023+0038 During a Low-Mass X-ray Binary State

Amruta Jaodand, Anne M. Archibald, Jason W. T. Hessels +5

Transitional millisecond pulsars (tMSPs) switch, on roughly multi-year timescales, between rotation-powered radio millisecond pulsar (RMSP) and accretion-powered low-mass X-ray bin…