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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
Supernovae with Two Peaks in the Optical Light Curve and the Signature of Progenitors with Low-mass Extended Envelopes
Ehud Nakar,Anthony L. Piro +1 more
TL;DR: In this paper, it was shown that a standard progenitor cannot produce a double-peaked light curve in the $R$ and $I$ bands, and cannot exhibit a fast drop in the bolometric luminosity as is seen after the first peak.
Proceedings ArticleDOI
The Turbulent Story of X‐ray Bursts: Effects of Shear Mixing on Accreting Neutron Stars
Anthony L. Piro,Lars Bildsten +1 more
TL;DR: In this paper, the authors studied the impact of mixing on the performance of X-ray bursts in a differentially rotating neutron star and found that mixing has the greatest impact when the buoyancy at the compositional discontinuity between accreted matter and ashes is overcome.
Journal ArticleDOI
Unstable Nonradial Oscillations on Helium Burning Neutron Stars
Anthony L. Piro,Lars Bildsten +1 more
TL;DR: In this paper, the authors analyzed the stability of nonradial oscillations, finding one unstable mode for pure helium accretion, which is a shallow surface wave which resides in the helium atmosphere above the heavier ashes of the ocean.
Posted Content
The Spreading Layer and Dwarf Nova Oscillations
Anthony L. Piro,Lars Bildsten +1 more
TL;DR: In this article, the authors describe the spreading layer model of a white dwarf surface and propose that such a model can explain the sensitivity of DNOs to accretion rate. But the model is not suitable for the detection of dwarf novae, symbiotic binaries, and supersoft sources.