Showing 1–20 of 106 results
/ Date/ Name
Mar 14, 2023Photometry and spectroscopy of the Type Icn supernova 2021ckj: The diverse properties of the ejecta and circumstellar matter of Type Icn SNeMar 22, 2024Including a Luminous Central Remnant in Radiative Transfer Simulations for Type Iax SupernovaeAug 11, 2023Unprecedented early flux excess in the hybrid 02es-like type Ia supernova 2022ywc indicates interaction with circumstellar materialFeb 3, 2022Modelling the spectra of the kilonova AT2017gfo -- I: The photospheric epochsJul 31, 2012Synthetic X-ray spectra for simulations of the dynamics of an accretion flow irradiated by a quasarOct 11, 2011Analytical approximations to numerical solutions of theoretical emission measure distributionsOct 18, 20123D deflagration simulations leaving bound remnants: a model for 2002cx-like Type Ia supernovaeDec 12, 2018Progenitor candidate for the type II-P supernova SN 2018aoq in NGC 4151Feb 5, 2019Spectral sequences of Type Ia supernovae. II. Carbon as a diagnostic tool for explosion mechanismsDec 20, 2018Detecting the signatures of helium in type Iax supernovaeSep 7, 2021Type Iax supernovae from deflagrations in Chandrasekhar mass white dwarfsApr 19, 2016The peculiar Type Ia supernova iPTF14atg: Chandrasekhar-mass explosion or violent merger?Jul 26, 2017Spectral sequences of Type Ia supernovae. I. Connecting normal and sub-luminous SN Ia and the presence of unburned carbonMay 20, 2015Constraints on explosive silicon burning in core-collapse supernovae from measured Ni/Fe ratiosMar 11, 2015On the diversity of super-luminous supernovae: ejected mass as the dominant factorAug 3, 20052-D Monte Carlo simulations of H I line formation in massive YSO disk windsJun 2, 2005Modelling the chromosphere and transition region of Epsilon Eri (K2 V)Oct 4, 2004Modelling the X-ray spectra of high velocity outflows from quasarsMar 27, 2018Using late-time optical and near-infrared spectra to constrain Type Ia supernova explosion propertiesFeb 13, 2007Off-center explosions of Chandrasekhar-mass white dwarfs: an explanation of super-bright type Ia supernovae?