activity
20132026
most citedThe NewAthena mission concept in the context of the next decade of X-ray astronomy

106 citations · 331 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2026★ 3 cited

Periodic Radio and X-ray Emission from an Accreting White Dwarf Binary

Kovi Rose, Joshua Pritchard, Tara Murphy +26

Long period radio transients (LPTs) are coherent bursts of polarised radio emission that repeat periodically on timescales of minutes to hours. Little is known about the physical o…

astro-ph.IM2025★ 106 cited

The NewAthena mission concept in the context of the next decade of X-ray astronomy

Mike Cruise, Matteo Guainazzi, James Aird +16

Large X-ray observatories such as Chandra and XMM-Newton have been delivering scientific breakthroughs in research fields as diverse as our Solar System, the astrophysics of stars,…

astro-ph.HE2024★ 4 cited

Polarized multiwavelength emission from pulsar wind - accretion disk interaction in a transitional millisecond pulsar

M. C. Baglio, F. Coti Zelati, A. Di Marco +17

Transitional millisecond pulsars (tMSPs) bridge the evolutionary gap between accreting neutron stars in low-mass X-ray binaries and millisecond radio pulsars. These systems exhibit…

astro-ph.HE2024★ 1 cited

Constraints on the dense matter equation of state from young and cold isolated neutron stars

Alessio Marino, Clara Dehman, Konstantinos Kovlakas +3

Neutron stars are the dense and highly magnetic relics of supernova explosions of massive stars. The quest to constrain the Equation of State (EoS) of ultra-dense matter and thereb…

astro-ph.HE2024★ 19 cited

3D code for MAgneto-Thermal evolution in Isolated Neutron Stars, MATINS: thermal evolution and lightcurves

Stefano Ascenzi, Daniele Viganò, Clara Dehman +3

The thermal evolution of isolated neutron stars is a key element in unraveling their internal structure and composition and establishing evolutionary connections among different ob…

astro-ph.SR2015★ 51 cited

Simulated magnetic field expulsion in neutron star cores

J. G. Elfritz, J. A. Pons, N. Rea +2

The study of long-term evolution of neutron star (NS) magnetic fields is key to understanding the rich diversity of NS observations, and to unifying their nature despite the differ…

astro-ph.HE2015★ 87 cited

Constraining the GRB-magnetar model by means of the Galactic pulsar population

Nanda Rea, Miguel Gullon, Jose' A. Pons +4

A large fraction of Gamma Ray Bursts (GRBs) displays an X-ray plateau phase within <10^{5} s from the prompt emission, proposed to be powered by the spin-down energy of a rapidly s…

astro-ph.HE2015★ 56 cited

Population Synthesis of Isolated Neutron Stars with magneto-rotational evolution II: from radio-pulsars to magnetars

M. Gullón, J. A. Pons, J. A. Miralles +3

Population synthesis studies constitute a powerful method to reconstruct the birth distribution of periods and magnetic fields of the pulsar population. When this method is applied…

astro-ph.HE2015

Magnetic fields in Neutron Stars

Daniele Viganò, Jose A. Pons, Juan A. Miralles +1

Isolated neutron stars show a diversity in timing and spectral properties, which has historically led to a classification in different sub-classes. The magnetic field plays a key r…

astro-ph.HE2013★ 4 cited

Magnetic fields in neutron stars

Daniele Viganò

This work aims at studying how magnetic fields affect the observational properties and the long-term evolution of isolated neutron stars, which are the strongest magnets in the uni…