collaborators

7 papers

astro-ph.HE2026

The first IXPE view of the eclipsing ADC source 4U 1822-37

A. Anitra, A. Gnarini, T. Di Salvo +16

Accretion-disc corona sources are high-inclination low-mass X-ray binaries in which the innermost regions are hidden and the observed X-ray emission is dominated by radiation scatt…

astro-ph.HE2026

XRISM/Resolve observations of Hercules X-1: a pulsating, highly broadened Fe K emission line from the neutron star accretion column

Peter Kosec, Laura Brenneman, Erin Kara +11

The study of X-ray pulsar accretion columns helps us characterize accretion physics in this extreme regime of strong gravity and strong magnetic fields. Previous observations of th…

astro-ph.HE2026

XRISM/Resolve observations of Hercules X-1: vertical structure and kinematics of the disk wind

Peter Kosec, Laura Brenneman, Erin Kara +11

X-ray binary accretion disk winds can carry away a significant fraction of the matter transferred from the companion and hence strongly affect the accretion flow and the long-term…

astro-ph.HE2025

XMM-Newton multi-year campaign on NGC 55 ULX-1: Resolving the wind and its variability with RGS

C. Pinto, S. Caserta, F. Barra +12

Winds are an important ingredient in the evolution of X-ray binary (XRB) systems, particularly those at high accretion rates such as ultra-luminous X-ray sources (ULXs), because th…

astro-ph.HE2025

A mysterious feature in the NICER spectrum of 4U 1820-30: A gravitationally redshifted absorption line?

R. Iaria, T. Di Salvo, A. Anitra +6

A mysterious absorption feature at approximately 3.8 keV has been identified in the NICER spectrum of the low-mass X-ray binary system 4U 1820-30. We interpret this feature as a gr…

astro-ph.HE2025

A new pulsating neutron star in the Ultraluminous X-ray source NGC 4559 X7?

F. Pintore, C. Pinto, G. Rodriguez-Castillo +17

Ultraluminous X-ray sources (ULX) are extragalactic objects with X-ray luminosities above the Eddington limit for a 10 Msun black hole (BH). ULXs may host super-Eddington accreting…