820 citations · 11.6k across the 267 of their papers we have counts for
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Dust destruction in non-radiative shocks
H. Zhu, P. Slane, J. Raymond +1
Supernova remnant (SNR) shock waves are the main place where interstellar dust grains are destroyed. However, the dust destruction efficiency in non-radiative shocks is still not w…
Probing the Innermost Ejecta Layers in SNR Kes 75: Implications for the Supernova Progenitor
Tea Temim, Patrick Slane, Tuguldur Sukhbold +3
Supernova remnants (SNRs) that contain pulsar wind nebulae (PWNe) are characterized by distinct evolutionary stages. In very young systems, the PWN drives a shock into the innermos…
An Ejecta Kinematics Study of Kepler's Supernova Remnant with High-Resolution HETG Spectroscopy
Matthew J. Millard, Jayant Bhalerao, Sangwook Park +6
We report our measurements of the bulk radial velocity from a sample of small, metal-rich ejecta knots in Kepler's Supernova Remnant (SNR). We measure the Doppler shift of the He-l…
Astro2020 Science White Paper: Future X-ray Studies of Supernova Remnants
Brian J. Williams, Katie Auchettl, Carles Badenes +13
This is a white paper submitted in response to the call from the Astro2020 Decadal Survey Committee. We outline the scientific progress that will be made in the next few decades in…
Supernova Remnants in High Definition
Laura A. Lopez, Brian J. Williams, Samar Safi-Harb +14
Supernova remnants (SNRs) offer the means to study SN explosions, dynamics, and shocks at sub-parsec scales. X-ray observations probe the hot metals synthesized in the explosion an…