most citedPulsars and Millisecond Pulsars I: Advancements, Open Questions and finding Gaps via statistical insights

3 citations · 8 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2026

Dynamical Preconditions for Ice Formation in Supernova Remnant and Cloud Interactions: A 2D MHD Study

A. Yeghikyan, M. Rah, S. Shamyar +1

Water ice has been detected in several supernova remnants despite the strong heating and radiation in these environments. This challenges standard expectations for dust survival. U…

astro-ph.HE2026★ 2 cited

Dust and Ices in the SNR

A. Yeghikyan, M. Rah, S. Shamyar

The presence of dust in supernova remnants (SNRs) is confirmed by extensive infrared data from observatories such as Spitzer, Herschel, and JWST, alongside theoretical models of du…

astro-ph.HE2026★ 1 cited

Pulsars and Millisecond Pulsars III: Tracing Compact Object Dynamics in Globular Clusters with NBODY6++GPU

M. Rah, R. Spurzem, F. Flammini Dotti +1

Neutron stars in globular clusters follow complex evolutionary pathways shaped by binary interactions, mass transfer, and dynamical exchanges. Direct N-body simulations such as NBO…

astro-ph.HE2026★ 2 cited

Pulsars and Millisecond Pulsars II: Deep diving into the Evolutionary Mechanisms

Maria Rah, Rainer Spurzem, Francesco Flammini Dotti +1

This second paper in our series investigates the evolutionary mechanisms that shape pulsars and millisecond pulsars (MSPs) across different astrophysical environments. We focus on…

astro-ph.HE2026★ 3 cited

Pulsars and Millisecond Pulsars I: Advancements, Open Questions and finding Gaps via statistical insights

Maria Rah, Areg Mickaelian, Francesco Flammini Dotti +1

We present a statistical study of pulsars and millisecond pulsars (MSPs) based on multiwavelength observations in the Galactic Field and Globular Clusters. We examine their emissio…

astro-ph.GA2024

Unraveling the Origins and Development of the Galactic Disk through Metal-Poor Stars

Maria Rah, Manolya Yatman, Ali Taani +2

The Milky Way is a spiral galaxy comprising three main components: the Bulge, the Disk, and the Halo. Of particular interest is the Galactic disk, which holds a significant portion…