Type Ia supernovae (SNe Ia) are important distance indicators, element factories, cosmic-ray
accelerators, kinetic-energy sources in galaxy evolution, and end points of stellar binary …

A concise and critical review of Balmer-dominated shocks (BDSs) is presented, summarizing
the state of theory and observations, including models with/without shock precursors and …

ABSTRACT We report unique Expanded Very Large Array observations of SN 2011fe
representing the most sensitive radio study of a Type Ia supernova to date. Our data place …

ABSTRACT SN 2006tf is the third most luminous supernova (SN) discovered so far, after SN
2005ap and SN 2006gy. SN 2006tf is valuable because it provides a link between two …

We introduce a deep (670 ks) X-ray survey of the entire SN 1006 remnant from the Chandra
X-Ray Observatory, together with a deep Hα image of SN 1006 from the 4 m Blanco …

Using radio, X-ray, and optical observations, we present evidence for morphological
changes due to efficient cosmic ray ion acceleration in the structure of the southeastern …

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

We report new H i observations of the Type Ia supernova remnant (SNR) SN 1006 using the
Australia Telescope Compact Array with an angular resolution of $4\buildrel {\,\prime}\over …

The interaction of a shock with a cloud has been extensively studied in the literature, where
the effects of magnetic fields, radiative cooling and thermal conduction have been …

We report on the proper motions of Balmer-dominated filaments in Kepler's supernova
remnant using high resolution images obtained with the Hubble Space Telescope at two …