activity
20242026
collaborators

5 papers

astro-ph.HE2026

Spectroscopic modeling of ionic structure in stellar winds of high-mass X-ray binaries

G. Sanjurjo-Ferrín, V. Grinberg, I. El Mellah +6

High-mass X-ray binaries (HMXBs) provide a natural laboratory to study radiatively driven stellar winds under strong external X-ray irradiation. As the compact object moves along i…

astro-ph.HE2026

Predictions for the X-ray polarisation modulation in Cygnus X-1 from reflection off the stellar companion and its wind

Bert Vander Meulen, Kun Hu, Victoria Grinberg +1

Context. Cyg X-1 is one of the brightest X-ray binaries and has been observed multiple times with the Imaging X-ray Polarimetry Explorer (IXPE). Recent studies report tentative evi…

astro-ph.HE2025

Pulse profile variations in the accreting X-ray pulsar Vela X-1

V. Madurga-Favieres, A. Martin-Carrillo, C. M. Diez +7

Vela X-1 is a well-studied accreting X-ray pulsar, with a distinctive pulse profile that has been found to be very similar in different observations spread out over decades. On the…

astro-ph.HE2025

Low-frequency spectra of neutron star + OB supergiant binaries: Does wind density drive persistent and flaring modes of accretion?

J. van den Eijnden, L. Sidoli, M. Díaz Trigo +10

Neutron star high-mass X-ray binaries are well-studied in wavebands between the infrared and hard X-rays. Their low-frequency millimeter and radio properties, on the other hand, re…

astro-ph.HE2024

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…