118 citations · 189 across the 5 of their papers we have counts for
5 papers
Chandra reveals a possible ultra-fast outflow in the super-Eddington Be/X-ray binary Swift J0243.6+6124
J. van den Eijnden, N. Degenaar, N. S. Schulz +8
Accretion at super-Eddington rates is expected to be accompanied by strong outflows. Such outflows are observed in Galactic X-ray binaries and extragalactic Ultra-luminous X-ray so…
Vela X-1 as a laboratory for accretion in High-Mass X-ray Binaries
P. Kretschmar, S. Martínez-Núñez, F. Fürst +7
Vela X-1 is an eclipsing high mass X-ray binary (HMXB) consisting of a 283s accreting X-ray pulsar in a close orbit of 8.964 days around the B0.5Ib supergiant HD77581 at a distance…
Radio emission from the X-ray pulsar Her X-1: a jet launched by a strong magnetic field neutron star?
J. van den Eijnden, N. Degenaar, T. D. Russell +5
Her X-1 is an accreting neutron star in an intermediate-mass X-ray binary. Like low-mass X-ray binaries (LMXBs), it accretes via Roche-lobe overflow, but similar to many high-mass…
Discovery of radio emission from the symbiotic X-ray binary system GX 1+4
J. van den Eijnden, N. Degenaar, T. D. Russell +5
We report the discovery of radio emission from the accreting X-ray pulsar and symbiotic X-ray binary GX 1+4 with the Karl G. Jansky Very Large Array. This is the first radio detect…
Inclination dependence of QPO phase lags in black hole X-ray binaries
J. van den Eijnden, A. Ingram, P. Uttley +3
Quasi-periodic oscillations (QPOs) with frequencies from - Hz are a common feature in the X-ray emission of accreting black hole binaries. As the QPOs originate from…