L. Tomasella

7 ta ish

Astronomical Observatory of Padova

1. Gaia17biu/SN 2017egm in NGC 3191: The Closest Hydrogen-poor Superluminous Supernova to Date Is in a “Normal,” Massive, Metal-rich Spiral Galaxy

   S. Bose, Subo Dong, A. Pastorello +55

   MaqolaOAOchiq kirish20183 iqtibos

   ABIABI:AkademIndex/2026.other.088107

2. Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger

   E. Pian, P. D’Avanzo, S. Benetti +81

   Maqola20173 iqtibos

   ABIABI:AkademIndex/2026.other.351200

3. Slowly fading super-luminous supernovae that are not pair-instability explosions

   M. Nicholl, Stephen Smartt, Anders Jerkstrand +57

   MaqolaOAOchiq kirish20132 iqtibos

   ABIABI:AkademIndex/2026.other.212813

4. Observations of the very young Type Ia Supernova 2019np with early-excess emission

   Hanna Sai, Xiaofeng Wang, N. Elias–Rosa +30

   Maqola20222 iqtibos

   ABIABI:AkademIndex/2026.other.252767

5. A comparison between short GRB afterglows and kilonova AT2017gfo: shedding light on kilonovae properties

   A. Rossi, G. Stratta, E. Maiorano +26

   Maqola20202 iqtibos

   ABIABI:AkademIndex/2026.other.345001

6. SN 2022vqz: a peculiar subluminous Type Ia supernova with prominent early excess emission

   Gaobo Xi, Xiaofeng Wang, Gaici Li +22

   MaqolaOAOchiq kirishGamma-ray bursts and supernovaeMonthly Notices of the Royal Astronomical Society20230 iqtibos

   ABIABI:AkademIndex/2023.article.000786

7. SN 2022vqz: A Peculiar Subluminous Type Ia Supernova with Prominent Early Excess Emission

   Gaobo Xi, Xiaofeng Wang, Gaici Li +22

   Preprint20230 iqtibos

   ABIABI:AkademIndex/2023.preprint.000277