Showing 1–20 of 20 results
/ Date/ Name
Oct 17, 2025Production of radioactive $^{22}$Na in core-collapse supernovae: the Ne-E(L) component in presolar grains and its possible consequences on supernova observationsJun 6, 2024Shockingly Bright Warm Carbon Monoxide Molecular Features in the Supernova Remnant Cassiopeia A Revealed by JWSTJul 5, 2023JWST detection of heavy neutron capture elements in a compact object mergerMay 16, 2022Horizons: Nuclear Astrophysics in the 2020s and BeyondNov 11, 2021The Gamow Explorer: A gamma-ray burst observatory to study the high redshift universe and enable multi-messenger astrophysicsOct 29, 2021Multi-messenger-Athena Synergy White PaperAug 19, 2020The Broad-band Counterpart of the Short GRB 200522A at $z=0.5536$: A Luminous Kilonova or a Collimated Outflow with a Reverse Shock?Mar 11, 2019Gamma Rays and Gravitational WavesMar 11, 2019Opportunities for Multimessenger Astronomy in the 2020sDec 19, 2018Remnants and ejecta of thermonuclear electron-capture supernovae: Constraining oxygen-neon deflagrations in high-density white dwarfsSep 25, 2017NuGrid Stellar Data Set. II. Stellar Yields from H to Bi for Stellar Models with Mzams = 1 to 25Msun and Z = 0.0001 to 0.02Jun 13, 2017Microlensing constraints on the mass of single stars from HST astrometric measurementsOct 26, 2015H ingestion into He-burning convection zones in super-AGB stellar models as a potential site for intermediate neutron-density nucleosynthesisMay 27, 2014Double Compact Objects III: Gravitational Wave Detection RatesMar 14, 2013Production of carbon-rich presolar grains from massive starsDec 17, 2012The 12C + 12C reaction and the impact on nucleosynthesis in massive starsJan 5, 2012The effect of 12C + 12C rate uncertainties on the evolution and nucleosynthesis of massive starsFeb 15, 2010The effect of 12C + 12C rate uncertainties on s-process yieldsFeb 19, 2009What Are Gamma-Ray Bursts -- The Unique Role of Very High Energy Gamma-Ray ObservationsOct 2, 2008Gamma Ray Burst Section of the White Paper on the Status and Future of Ground-based TeV Gamma-ray Astronomy