Results 71 to 80 of about 118 (100)

ANALYTIC SOLUTION FOR SELF-REGULATED COLLECTIVE ESCAPE OF COSMIC RAYS FROM THEIR ACCELERATION SITES. [PDF]

Astrophys J, 2013
Malkov MA, Diamond PH, Sagdeev RZ, Aharonian FA, Moskalenko IV.   +4 more
europepmc   +1 more source

Discrete effects in stellar feedback: Individual Supernovae, Hypernovae, and IMF Sampling in Dwarf Galaxies. [PDF]

Mon Not R Astron Soc, 2018
Su KY, Hopkins PF, Hayward CC, Ma X, Boylan-Kolchin M, Kasen D, Kereš D, Faucher-Giguère CA, Orr ME, Wheeler C.   +9 more
europepmc   +1 more source

Cosmic-Ray Propagation in Light of the Recent Observation of Geminga. [PDF]

Astrophys J, 2019
Jóhannesson G, Porter TA, Moskalenko IV.   +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, Thomas AM, Dangi BB, Kaiser RI, Mebel AM, Millar TJ.   +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.
europepmc   +1 more source

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, Jóhannesson G, Moskalenko IV.   +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, Digel SW, Casandjian JM, Franckowiak A, Grenier IA, Jóhannesson G, Marshall DJ, Moskalenko IV, Negro M, Orlando E, Porter TA, Reimer O, Strong AW.   +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

X-ray studies of supernova remnants: A different view of supernova explosions [PDF]

Proceedings of the National Academy of Sciences of the United States of America, 2010
Carles Badenes
exaly   +2 more sources

Some of the next articles are maybe not open access.

Related searches:

First Results from ISO Spectra of Supernova Remnants Heavily Interacting with the ISM

Astrophysics and Space Science, 1997
ISO 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
E. Oliva, S. Drapatz, D. Lutz, E. Sturm, A. F. M. Moorwood   +4 more
openaire   +1 more source