activity
20192026
most citedRevisiting the archetypical wind accretor Vela X-1 in depth -- A case study of a well-known X-ray binary and the limits of our knowledge

46 citations · 142 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2026

Jet launching from the Kerr black hole magnetosphere: An electrogeodesic approach

Jibril Ben Achour, Ileyk El Mellah, Eric Gourgoulhon

The launch of relativistic jets of plasma on astrophysical to cosmological scales is observed in a variety of astrophysical sources, from active galactic nuclei to X-ray binaries.…

astro-ph.HE2024★ 5 cited

Variable structures in the stellar wind of the HMXB Vela X-1

L. Abalo, P. Kretschmar, F. Fürst +9

Strong stellar winds are an important feature in wind-accreting high-mass X-ray binary (HMXB) systems, providing insights into stellar evolution and their impact on surrounding env…

astro-ph.HE2021★ 46 cited

Revisiting the archetypical wind accretor Vela X-1 in depth -- A case study of a well-known X-ray binary and the limits of our knowledge

Peter Kretschmar, Ileyk El Mellah, Silvia Martínez-Núñez +9

Context: Vela X-1 is one of the best studied X-ray binaries. Frequently though, specific values for its parameters have been used in subsequent studies without considering alternat…

astro-ph.SR2020★ 42 cited

Wind morphology around cool evolved stars in binaries: the case of slowly accelerating oxygen-rich outflows

I. El Mellah, J. Bolte, L. Decin +2

The late stellar evolutionary phases of low and intermediate-mass stars are strongly constrained by their mass-loss rates. The wind surrounding cool evolved stars frequently shows…

astro-ph.HE2019★ 5 cited

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…

astro-ph.HE2019★ 2 cited

Variability in high-mass X-ray binaries

F. Fuerst, P. Kretschmar, V. Grinberg +5

Strongly magnetized, accreting neutron stars show periodic and aperiodic variability over a wide range of time scales. By obtaining spectral and timing information on these differe…

astro-ph.SR2019★ 42 cited

Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction

L. Decin, W. Homan, T. Danilovich +12

In 1981, the idea of a superwind that ends the life of cool giant stars was proposed. Extreme OH/IR-stars develop superwinds with the highest mass-loss rates known so far, up to a…