Cosmic-Ray Propagation in Light of the Recent Observation of Geminga. [PDF]
Astrophys J, 2019 Jóhannesson G +2 more
europepmc +1 more source
Directed gas phase formation of silicon dioxide and implications for the formation of interstellar silicates. [PDF]
Nat Commun, 2018 Yang T +5 more
europepmc +1 more source
The γ-ray afterglows of tidal disruption events. [PDF]
Mon Not R Astron Soc, 2016 Chen X, Gómez-Vargas GA, Guillochon J.
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High-energy Gamma Rays from the Milky Way: Three-dimensional Spatial Models for the Cosmic-Ray and Radiation Field Densities in the Interstellar Medium. [PDF]
Astrophys J, 2017 Porter TA +2 more
europepmc +1 more source
FERMI-LAT OBSERVATIONS OF HIGH- AND INTERMEDIATE-VELOCITY CLOUDS: TRACING COSMIC RAYS IN THE HALO OF THE MILKY WAY. [PDF]
Astrophys J, 2015 Tibaldo L +12 more
europepmc +1 more source
Magnetic fields in non-convective regions of stars. [PDF]
R Soc Open Sci, 2017 Braithwaite J, Spruit HC.
europepmc +1 more source
Triggered Star Formation inside the Shell of a Wolf-Rayet Bubble as the Origin of the Solar System. [PDF]
Astrophys J, 2017 Dwarkadas VV +4 more
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The Evolution of Compact Binary Star Systems. [PDF]
Living Rev Relativ, 2014 Postnov KA, Yungelson LR.
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First Results from ISO Spectra of Supernova Remnants Heavily Interacting with the ISM
Astrophysics and Space Science, 1997ISO spectra1 of the supernova remnant RCW103 are presented. This object is the prototype of a SNR shock heavily interacting with dense ISM (probably a molecular cloud). The spectra are dominated by prominent lines and show very little continuum at » < 40 µm suggesting that the 12 and 25 µm IRAS emission from these types of remnant could be dominated by
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