The high energy X-ray probe (HEX-P): a new window into neutron star accretion

The high energy X-ray probe (HEX-P): a new window into neutron star accretion

Accreting neutron stars (NSs) represent a unique laboratory for probing the physics of accretion in the presence of strong magnetic fields (B ≳ 108 G). Additionally, the matter inside the NS itself exists in an ultra-dense, cold state that cannot be reproduced in Earth-based laboratories. Hence, obs...

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Bibliographic Details
Main Authors: R. M. Ludlam, C. Malacaria, E. Sokolova-Lapa, F. Fuerst, P. Pradhan, A. W. Shaw, K. Pottschmidt, S. Pike, G. Vasilopoulos, J. Wilms, J. A. García, K. Madsen, D. Stern, C. Maitra, M. Del Santo, D. J. Walton, M. C. Brumback, J. van den Eijnden
Format: Article
Language:English
Published: Frontiers Media S.A. 2023-12-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
neutron stars
accretion
high-mass X-ray binary stars
low-mass X-ray binary stars
magnetic fields
high energy astrophysics
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2023.1292500/full

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