activity
20052009
most citedSpatial Structure and Collisionless Electron Heating in Balmer-dominated Shocks

110 citations · 323 across the 9 of their papers we have counts for

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9 papers · 1 filter

astro-ph200816 cited

A Direct Measurement of the Dust Extinction Curve in an Intermediate-Redshift Galaxy

Kevin Heng, Davide Lazzati, Rosalba Perna +5

We present a proof-of-concept study that dust extinction curves can be extracted from the infrared (IR), optical, ultraviolet (UV) and X-ray afterglow observations of GRBs without…

astro-ph2008110 cited

Spatial Structure and Collisionless Electron Heating in Balmer-dominated Shocks

Matthew van Adelsberg, Kevin Heng, Richard McCray +1

Balmer-dominated shocks in supernova remnants (SNRs) produce strong hydrogen lines with a two-component profile composed of a narrow contribution from cold upstream hydrogen atoms,…

astro-ph200728 cited

Probing Elemental Abundances in SNR 1987A Using XMM-Newton

Kevin Heng, Frank Haberl, Bernd Aschenbach +1

We report on the latest (2007 Jan) observations of supernova remnant (SNR) 1987A from the XMM-Newton mission. Since the 2003 May observations of Haberl et al. (2006), 11 emission l…

astro-ph200729 cited

Broad Lyman-Alpha Emission from Supernova Remnants in Young Galaxies

Kevin Heng, Rashid Sunyaev

Charge transfer (or exchange) reactions between hydrogen atoms and protons in collisionless shocks of supernova remnants (SNRs) are a natural way of producing broad Balmer, Lyman a…

astro-ph200734 cited

The Transition Zone in Balmer-Dominated Shocks

Kevin Heng, Matthew van Adelsberg, Richard McCray +1

We examine the structure of the post-shock region in supernova remnants (SNRs). The ``shock transition zone'' is set up by charge transfer and ionization events between atoms and i…

astro-ph20071 cited

The Reverse Shock of SNR 1987A

Kevin Heng

The reverse shock of supernova remnant (SNR) 1987A emits in H-alpha and Ly-alpha, and comes in two flavors: surface and interior. The former is due to direct, impact excitation of…