EDUARDO
BRAVO GUIL
COLABORADOR EXTRAORDINARIO
University of Pittsburgh
Pittsburgh, Estados UnidosPublicaciones en colaboración con investigadores/as de University of Pittsburgh (12)
2022
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Stable nickel production in type Ia supernovae: A smoking gun for the progenitor mass?
Astronomy and Astrophysics, Vol. 660
2020
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A Nucleosynthetic Origin for the Southwestern Fe-rich Structure in Kepler's Supernova Remnant
Astrophysical Journal, Vol. 890, Núm. 2
2019
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SNR-calibrated Type Ia supernova models
Monthly Notices of the Royal Astronomical Society, Vol. 482, Núm. 4, pp. 4346-4363
2018
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Chandrasekhar and Sub-Chandrasekhar Models for the X-Ray Emission of Type Ia Supernova Remnants. I. Bulk Properties
Astrophysical Journal, Vol. 865, Núm. 2
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Evidence for a Sub-Chandrasekhar-mass Type Ia Supernova in the Ursa Minor Dwarf Galaxy
Astrophysical Journal, Vol. 857, Núm. 2
2017
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Observational evidence for high neutronization in supernova remnants: implications for type ia supernova progenitors
Astrophysical Journal, Vol. 843, Núm. 1
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THE ORIGIN of the IRON-RICH KNOT in TYCHO'S SUPERNOVA REMNANT
Astrophysical Journal, Vol. 834, Núm. 2
2016
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Gamma-ray emission from SN2014J near maximum optical light
Astronomy and Astrophysics, Vol. 588
2015
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A chandrasekhar mass progenitor for the Type Ia supernova remnant 3C 397 from the enhanced abundances of nickel and manganese
Astrophysical Journal Letters, Vol. 801, Núm. 2
2013
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A super-solar metallicity for the progenitor of Kepler's supernova
Astrophysical Journal Letters, Vol. 767, Núm. 1
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Observation of SN2011fe with INTEGRAL: I. Pre-maximum phase
Astronomy and Astrophysics, Vol. 552
2012
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Observations of SN2011fe with INTEGRAL
Proceedings of Science