output
19922026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2014 · astro-ph.HEShow all

42 papers · 2 filters

astro-ph.HE2014★ 6 cited

Numerical Simulations of Mach Stem Formation via Intersecting Bow Shocks

Edward C. Hansen, Adam Frank, Patrick Hartigan

Hubble Space Telescope observations show bright knots of H emission within outflowing young stellar jets. Velocity variations in the flow create secondary bow shocks that may in…

astro-ph.HE2014★ 28 cited

The Hard X-Ray View of the Young Supernova Remnant G1.9+0.3

Andreas Zoglauer, Stephen P. Reynolds, Hongjun An +12

NuSTAR observed G1.9+0.3, the youngest known supernova remnant in the Milky Way, for 350 ks and detected emission up to 30 keV. The remnant's X-ray morphology does not change…

astro-ph.HE2014★ 27 cited

Finding the First Cosmic Explosions. IV. 90 - 140 M Pair-Instability Supernovae

Joseph Smidt, Daniel J. Whalen, E. Chatzopoulos +4

Population III stars that die as pair-instability supernovae are usually thought to fall in the mass range of 140 - 260 M. But several lines of work have now shown that r…

astro-ph.HE2014★ 87 cited

Scaling of magnetic reconnection in relativistic collisionless plasmas

Yi-Hsin Liu, Fan Guo, William Daughton +2

Using fully kinetic simulations, we study the scaling of the inflow speed of collisionless magnetic reconnection from the non-relativistic to ultra-relativistic limit. In the anti-…

astro-ph.HE2014

Comparisons of Two- and Three-Dimensional Convection in Type I X-ray Bursts

M. Zingale, C. M. Malone, A. Nonaka +2

We perform the first detailed three-dimensional simulation of low Mach number convection preceding thermonuclear ignition in a mixed H/He X-ray burst. Our simulations include a mod…

astro-ph.HE2014★ 41 cited

Search for gamma-rays from the unusually bright GRB 130427A with the HAWC Gamma-ray Observatory

The HAWC collaboration, A. U. Abeysekara, R. Alfaro +90

The first limits on the prompt emission from the long gamma-ray burst (GRB) 130427A in the energy band are reported. GRB 130427A was the most powerful b…