collaborators

13 papers

astro-ph.HE2026

Superorbital variability in the quiescent black hole X-ray transient A0620-00

Enzo A. Saavedra, Roi Alonso, Teo Muñoz-Darias +10

Quiescent black hole low-mass X-ray binaries provide a key setting for probing accretion physics at low luminosities. A0620-00, the archetypal system in this class, has remained in…

astro-ph.SR2026

K 1-6 is a photoionised ISM nebula shaped by a fast-moving hot white dwarf in a triple system

Jaroslav Merc, David Jones, Ana Escorza +22

The study shows that nebula K 1‑6 is not a planetary nebula but interstellar gas photoionised by an evolved hot white dwarf, and that its central star is a hierarchical triple syst…

astro-ph.HE2026

Resolving SLX 1744-299 and SLX 1744-300 in the hard X-ray band: implications for their ultracompact nature

Enzo A. Saavedra, Montserrat Armas Padilla, Teo Muñoz-Darias

Persistent, low-luminosity low-mass X-ray binaries (LMXBs) offer a unique opportunity to study accretion in this poorly understood regime, as well as to unveil new members of the u…

astro-ph.HE2026

The NuSTAR view of Ultra-Compact X-ray Binaries

A. Borghese, M. Armas Padilla, T. Muñoz-Darias

Ultra-compact X-ray binaries (UCXBs) are a subclass of low-mass X-ray binaries (LMXBs) characterised by tight orbits and hydrogen-poor donor stars. We present a spectral and timing…

astro-ph.HE2026

Ubiquitous yet forgotten: broad absorptions in the optical spectra of low-mass X-ray binaries

D. Mata Sanchez, T. Munoz-Darias, J. Casares +2

Optical outburst spectra of low-mass X-ray binaries enable studies of extreme accretion and ejection phenomena. While some of their spectroscopic features have been analysed in det…

astro-ph.HE2025

The orbital period and inclination of the neutron star X-ray transient MAXI J1807+132

E. A. Saavedra, T. Muñoz-Darias, M. A. P. Torres +7

The neutron star X-ray transient MAXI J1807+132 has undergone outbursts in 2017, 2019, and 2023. We conducted an -band time series photometry campaign using the Isaac Newton Tel…