activity
20102026
most citedA Massive Pulsar in a Compact Relativistic Binary

3.9k citations · 8.9k across the 61 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

astro-ph.HE2020

Gaia pulsars and where to find them in EDR3

John Antoniadis

The Early Gaia Data Release 3 (EDR3) provides precise astrometry for nearly 1.5 billion sources across the entire sky. A few tens of these are associated with neutron stars in the…

astro-ph.HE2020★ 41 cited

Gaia pulsars and where to find them

John Antoniadis

While the majority of massive stars have a stellar companion, most pulsars appear to be isolated. Taken at face value, this suggests that most massive binaries break apart due to s…

astro-ph.HE2020★ 42 cited

A revisit of PSR J19093744 with 15-year high-precision timing

K. Liu, L. Guillemot, A. G. Istrate +10

We report on a high-precision timing analysis and an astrophysical study of the binary millisecond pulsar, PSR J19093744, motivated by the accumulation of data with well improve…

astro-ph.HE2020★ 34 cited

Measuring Interstellar Delays of PSR J0613-0200 over 7 years, using the Large European Array for Pulsars

R. A. Main, S. A. Sanidas, J. Antoniadis +19

Using data from the Large European Array for Pulsars (LEAP), and the Effelsberg telescope, we study the scintillation parameters of the millisecond pulsar J0613-0200 over a 7 year…

astro-ph.SR2020★ 49 cited

Pre-collapse Properties of Superluminous Supernovae and Long Gamma-Ray Burst Progenitor Models

David R. Aguilera-Dena, Norbert Langer, John Antoniadis +1

We analyze the properties of 42 rapidly rotating, low metallicity, quasi-chemically homogeneously evolving stellar models in the mass range between 4 and 45 at…

astro-ph.SR2020★ 21 cited

Type Ia supernovae from non-accreting progenitors

John Antoniadis, Savvas Chanlaridis, Götz Gräfener +1

Type Ia supernovae (SNe Ia) are manifestations of stars deficient of hydrogen and helium disrupting in a thermonuclear runaway. While explosions of carbon-oxygen white dwarfs are t…