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researcher

A. Piro

190 papers hereh-index 5413.5k citations277 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author12
  • first author27
  • middle author113
  • last author16

Across the 168 of 190 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE127
  • astro-ph.SR22
  • astro-ph20
  • astro-ph.EP8
  • astro-ph.CO7
  • astro-ph.IM4
same name
  • A. Piro — 1 paper, h 5
  • A. Piro — 1 paper, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20022026
most citedSwope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source

1.2k citations · 11.5k across the 187 of their papers we have counts for

collaborators
Showing 2011Show all

4 papers · 1 filter

astro-ph.HE2011★ 254 cited

Resonant Shattering of Neutron Star Crusts

David Tsang, Jocelyn S. Read, Tanja Hinderer +2

The resonant excitation of neutron star (NS) modes by tides is investigated as a source of short gamma-ray burst (sGRB) precursors. We find that the driving of a crust-core interfa…

astro-ph.SR2011★ 53 cited

Tidal Interactions in Merging White Dwarf Binaries

Anthony L. Piro

The recently discovered system J0651 is the tightest known detached white dwarf (WD) binary. Since it has not yet initiated Roche-lobe overflow, it provides a relatively clean envi…

astro-ph.HE2011★ 14 cited

G-Mode Excitation During the Pre-explosive Simmering of Type Ia Supernovae

Anthony L. Piro

Prior to the explosive burning of a white dwarf (WD) that makes a Type Ia supernova (SN Ia), the star "simmers" for ~10^3 yrs in a convecting, carbon burning region. I estimate the…

astro-ph.HE2011★ 119 cited

Supernova Fallback onto Magnetars and Propeller-Powered Supernovae

Anthony L. Piro, Christian D. Ott

We explore fallback accretion onto newly born magnetars during the supernova of massive stars. Strong magnetic fields (~10^{15} G) and short spin periods (~1-10 ms) have an importa…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.