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astro-ph200856 cited

Three-dimensional modeling of the asymmetric blast wave from the 2006 outburst of RS Ophiuchi: Early X-ray emission

S. Orlando, J. J. Drake, J. M. Laming

Chandra/HETG observations of the recurrent nova RS Ophiuchi at day 13.9 of its 2006 outburst reveal a spectrum covering a large range in plasma temperature and characterized by asy…

astro-ph200856 cited

The Heating of Thermal Electrons in Fast Collisionless Shocks: The Integral Role of Cosmic Rays

Cara E. Rakowski, J. Martin Laming, Parviz Ghavamian

Understanding the heating of electrons to quasi-thermal energies at collisionless shocks has broad implications for plasma astrophysics. It directly impacts the interpretation of X…

astro-ph200836 cited

Non-Maxwellian Proton Velocity Distributions in Nonradiative Shocks

J. C. Raymond, Philip A. Isenberg, J. M. Laming

The Balmer line profiles of nonradiative supernova remnant shocks provide the means to measure the post-shock proton velocity distribution. While most analyses assume a Maxwellian…

astro-ph2007151 cited

A Deep Chandra Observation of Kepler's Supernova Remnant: A Type Ia Event with Circumstellar Interaction

S. P. Reynolds, K. J. Borkowski, U. Hwang +4

We present initial results of a 750 ks Chandra observation of the remnant of Kepler's supernova of AD 1604. The strength and prominence of iron emission, together with the absence…

astro-ph2006211 cited

A Physical Relationship Between Electron-Proton Temperature Equilibration and Mach Number in Fast Collisionless Shocks

Parviz Ghavamian, J. Martin Laming, Cara E. Rakowski

The analysis of Balmer-dominated optical spectra from non-radiative (adiabatic) SNRs has shown that the ratio of the electron to proton temperature temperature at the blast wave is…

astro-ph2006156 cited

Collisional Ionization Equilibrium for Optically Thin Plasmas. I. Updated Recombination Rate Coefficients for Bare though Sodium-like Ions

P. Bryans, N. R. Badnell, T. W. Gorczyca +3

Reliably interpreting spectra from electron-ionized cosmic plasmas requires accurate ionization balance calculations for the plasma in question. However, much of the atomic data ne…