activity
20242026
collaborators

5 papers

astro-ph.HE2026

Optical transients from non-explosive double white-dwarf mergers: the case of a central neutron star remnant

M. M. Ridha Fathima, Alexandre M. R. Almeida, Mattia Bulla +3

Discoveries of ultra-massive magnetic white dwarfs (WDs) and peculiar pulsars have been proposed to originate in double white dwarf (DWD) mergers. There are three possible post-mer…

astro-ph.HE2026

Double White Dwarf Mergers as Progenitors of Long-Period Transients

Manuel Malheiro, Sarah V. Borges, Jaziel G. Coelho +6

There is an ongoing discussion in the literature on the nature of long-period transients (LPTs), radio-emitting sources with periods ranging from hundreds to tens of thousands of s…

astro-ph.HE2025

Short GRB 090510: a magnetized neutron star binary merger leading to a black hole

J. A. Rueda, R. Ruffini, Yu Wang

We model the short gamma-ray bursts (GRB) 090510 as the product of a magnetized neutron star (NS) binary merger. Accounting for the NS critical mass constraint given by the mass of…

astro-ph.HE2025

On the formation of strange quark stars from supernova in compact binaries

L. M. Becerra, F. Cipolletta, A. Drago +4

Strange quark stars (SQSs), namely compact stars entirely composed of deconfined quark matter, are characterized by similar masses and compactness to neutron stars (NSs) and have b…

astro-ph.HE2024

Can the central compact object in HESS J1731--347 be indeed the lightest neutron star observed?

Shu-Rui Zhang, Jorge A. Rueda, Rodrigo Negreiros

The exceptionally low mass of for the central compact object (CCO) XMMU J173203.3 -- 344518 (XMMU J1732) in the supernova remnant (SNR) HESS J1731 -…