A self-consistent model of cosmic ray transport in molecular clouds with ballistic, diffusive, and hybrid scenarios applied to Taurus shows enhanced scattering on clump scales, suppressed diffusion coefficients, and elevated ionization rates.
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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.
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Multiwavelength Probes of Cosmic Ray Transport in Molecular Cloud Structures
A self-consistent model of cosmic ray transport in molecular clouds with ballistic, diffusive, and hybrid scenarios applied to Taurus shows enhanced scattering on clump scales, suppressed diffusion coefficients, and elevated ionization rates.
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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.