Results 71 to 80 of about 113 (88)
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
europepmc +1 more source
The Evolution of Compact Binary Star Systems. [PDF]
Living Rev Relativ, 2014 Postnov KA, Yungelson LR.
europepmc +1 more source
Sub-arcsecond imaging of the water emission in Arp 220. [PDF]
Astron Astrophys, 2017 König S +16 more
europepmc +1 more source
The exceptional X-ray evolution of SN 1996cr in high resolution. [PDF]
Mon Not R Astron Soc, 2019 Quirola-Vásquez J +6 more
europepmc +1 more source
X-raying galaxies: a Chandra legacy. [PDF]
Proc Natl Acad Sci U S A, 2010 Wang QD.
europepmc +1 more source
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 +4 more
+4 more sources