X-ray luminous late-type giant binaries contribute ~20% of the GRXE continuum and ~40% of its iron line emission.
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3 Pith papers cite this work. Polarity classification is still indexing.
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New 2024 observations of NGC 3783 show the warm absorbers have 1.5 times higher total column density, with structural changes including a tripling in the dominant component, indicating significant evolution over 24 years.
Multi-mission X-ray imaging and spectroscopy of the PWN around PSR B1853+01 reveals a hard-spectrum outflow and diffuse halo interpreted as escaping high-energy particles.
citing papers explorer
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X-ray luminous late-type giants: an overlooked population contributing to the Galactic ridge iron line emission
X-ray luminous late-type giant binaries contribute ~20% of the GRXE continuum and ~40% of its iron line emission.
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Delving into the depths of NGC 3783 with XRISM: V. Broad-band modeling of ionized outflows
New 2024 observations of NGC 3783 show the warm absorbers have 1.5 times higher total column density, with structural changes including a tripling in the dominant component, indicating significant evolution over 24 years.
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The pulsar wind nebula around B1853+01 in X-rays
Multi-mission X-ray imaging and spectroscopy of the PWN around PSR B1853+01 reveals a hard-spectrum outflow and diffuse halo interpreted as escaping high-energy particles.