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High-mass X-ray binaries in the Milky WayX-ray broad-band study of the symbiotic X-ray binary 4U 1954+31The BeppoSAX view of the galactic high-mass X-ray binary 4U 0114+65IGR J16194-2810: a new symbiotic X-ray binaryULX spectra revisited: Accreting, highly magnetized neutron stars as the engines of ultraluminous X-ray sourcesLong-term evolution of the neutron-star spin period of SXP 1062
P2860
description
article publié dans la revue scientifique Astrophysical Journal
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im Oktober 2004 veröffentlichter wissenschaftlicher Artikel
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scientific article published in the Astrophysical Journal
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wetenschappelijk artikel
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наукова стаття, опублікована в жовтні 2004
@uk
name
Origin of the Soft Excess in X‐Ray Pulsars
@en
Origin of the Soft Excess in X‐Ray Pulsars
@nl
type
label
Origin of the Soft Excess in X‐Ray Pulsars
@en
Origin of the Soft Excess in X‐Ray Pulsars
@nl
prefLabel
Origin of the Soft Excess in X‐Ray Pulsars
@en
Origin of the Soft Excess in X‐Ray Pulsars
@nl
P356
P1476
Origin of the Soft Excess in X‐Ray Pulsars
@en
P2093
Ryan C. Hickox
Timothy R. Kallman
P304
P356
10.1086/423928
P407
P577
2004-10-20T00:00:00Z
P818
astro-ph/0407115
P819
2004ApJ...614..881H