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Anthony L. Piro
Researcher at Carnegie Institution for Science
Publications - 298
Citations - 14937
Anthony L. Piro is an academic researcher from Carnegie Institution for Science. The author has contributed to research in topics: Supernova & White dwarf. The author has an hindex of 62, co-authored 268 publications receiving 12532 citations. Previous affiliations of Anthony L. Piro include California Institute of Technology & Carnegie Learning.
Papers
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Journal ArticleDOI
Ca hnk: Calcium-rich transient SN 2016hnk from the helium shell detonation of a sub-chandrasekhar white dwarf
Wynn V. Jacobson-Galán,Wynn V. Jacobson-Galán,Abigail Polin,Abigail Polin,Ryan J. Foley,Georgios Dimitriadis,Charles D. Kilpatrick,Raffaella Margutti,David A. Coulter,Saurabh Jha,David O. Jones,Robert P. Kirshner,Yen-Chen Pan,Anthony L. Piro,Armin Rest,Armin Rest,César Rojas-Bravo +16 more
TL;DR: In this article, a Ca-rich supernova (SN 2016hnk) was modeled as a He-shell double-detonation explosion of a C/O white dwarf.
Journal ArticleDOI
Ultrahigh-Energy Cosmic Rays from the "En Caul" Birth of Magnetars
TL;DR: In this article, the authors explore whether the small amount of natal debris surrounding these magnetars allows the UHECRs to easily escape and investigate the impact of the unique environment around the magnetar, which consists of a bubble of relativistic particles and magnetic field within the debris.
Posted Content
Prompt Accretion Disk Formation in an X-Ray Faint Tidal Disruption Event
Tiara Hung,Ryan J. Foley,Enrico Ramirez-Ruiz,Jane L. Dai,Katie Auchettl,Charles D. Kilpatrick,Brenna Mockler,Jon Brown,David A. Coulter,Georgios Dimitriadis,Tom Holoien,Jamie Law-Smith,Anthony L. Piro,Armin Rest,César Rojas-Bravo,Matthew R. Siebert +15 more
TL;DR: In this article, the first unambiguous case of resolved double-peaked Balmer emission in a TDE has been detected in the ASASSN-18zj data set.
Journal ArticleDOI
The Fate of Neutron Star Binary Mergers
TL;DR: In this article, the authors combine relativistic calculations of NS masses using realistic EOSs with Monte Carlo population synthesis based on the mass distribution of NS binaries in our Galaxy to predict the distribution of fates expected.
Journal ArticleDOI
ASASSN-15pz: Revealing Significant Photometric Diversity among 2009dc-like, Peculiar SNe Ia
Ping Chen,Subo Dong,Boaz Katz,Christopher S. Kochanek,Juna A. Kollmeier,Kate Maguire,Kate Maguire,Mark M. Phillips,J. L. Prieto,J. L. Prieto,Benjamin J. Shappee,Maximilian Stritzinger,Subhash Bose,Peter J. Brown,Peter J. Brown,Thomas W.-S. Holoien,Lluís Galbany,Peter A. Milne,Nidia Morrell,Anthony L. Piro,Krzysztof Z. Stanek,Todd A. Thompson,Todd A. Thompson,David Young +23 more
TL;DR: In this article, the authors presented the results of the H2020 HST program of the European Organisation for Astronomical Research in the Southern Hemisphere, Chile under the ESO programme.