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most citedOverview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory

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astro-ph2008★ 82 cited

The End of Amnesia: A New Method for Measuring the Metallicity of Type Ia Supernova Progenitors Using Manganese Lines in Supernova Remnants

Carles Badenes, Eduardo Bravo, John P. Hughes

We propose a new method to measure the metallicity of Type Ia supernova progenitors using Mn and Cr lines in the X-ray spectra of young supernova remnants. We show that the Mn to C…

astro-ph2008★ 116 cited

Morphological evidence for azimuthal variations of the cosmic ray ion acceleration at the blast wave of SN 1006

Gamil Cassam-Chenai, John P. Hughes, Estela M. Reynoso +2

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 region…

astro-ph2008★ 85 cited

The Persistence of Memory, or How the X-Ray Spectrum of SNR 0509-67.5 Reveals the Brightness of its Parent Type Ia Supernova

Carles Badenes, John P. Hughes, Gamil Cassam-Chenai +1

We examine the dynamics and X-ray spectrum of the young Type Ia supernova remnant 0509-67.5 in the context of the recent results obtained from the optical spectroscopy of its light…

astro-ph2007★ 151 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-ph2007★ 169 cited

Are the Models for Type Ia Supernova Progenitors Consistent with the Properties of Supernova Remnants?

Carles Badenes, John P. Hughes, Eduardo Bravo +1

We explore the relationship between the models for progenitor systems of Type Ia supernovae and the properties of the supernova remnants that evolve after the explosion. Most model…

astro-ph2006★ 42 cited

Can Ejecta-Dominated Supernova Remnants be Typed from their X-ray Spectra? The Case of G337.2-0.7

Cara E. Rakowski, Carles Badenes, B. M. Gaensler +3

In this paper we use recent X-ray and radio observations of the ejecta-rich Galactic supernova remnant (SNR) G337.2-0.7 to determine properties of the supernova (SN) explosion that…