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20112025
most citedNumerical Relativity Simulations of the Neutron Star Merger GW170817: Long-Term Remnant Evolutions, Winds, Remnant Disks, and Nucleosynthesis

149 citations · 1.6k across the 58 of their papers we have counts for

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Showing 2017Show all

6 papers · 1 filter

astro-ph.GA2017★ 12 cited

Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts

Mohammadtaher Safarzadeh, Alexander P. Ji, Gregory A. Dooley +4

The smallest satellites of the Milky Way ceased forming stars during the epoch of reionization and thus provide archaeological access to galaxy formation at . Numerical studie…

astro-ph.GA2017★ 34 cited

The Fate of Gas rich Satellites in Clusters

Mohammadtaher Safarzadeh, Evan Scannapieco

We investigate the stellar mass loss of gas rich galaxies falling into clusters due to the change in the gravitational potential caused by the ram pressure stripping of their gas.…

astro-ph.GA2017★ 16 cited

On the Impact of Neutron Star Binaries Natal-Kick Distribution on the Galactic r-process Enrichment

Mohammadtaher Safarzadeh, Benoit Côté

We study the impact of the neutron star binaries' (NSBs) natal kick distribution on the Galactic r-process enrichment. We model the growth of a Milky Way type halo based on N-body…

astro-ph.GA2017★ 56 cited

Simulating Neutron Star Mergers as r-process Sources in Ultra Faint Dwarf Galaxies

Mohammadtaher Safarzadeh, Evan Scannapieco

To explain the high observed abundances of r-process elements in local ultra- faint dwarf (UFD) galaxies, we perform cosmological zoom simulations that include r-process production…

astro-ph.GA2017★ 15 cited

Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?

Mohammadtaher Safarzadeh, Yu Lu, Christopher C. Hayward

Matching the number counts and redshift distribution of submillimeter galaxies (SMGs) without invoking modifications to the initial mass function (IMF) has proved challenging for s…

astro-ph.HE2017★ 33 cited

Primordial black holes as seeds of magnetic fields in the universe

Mohammadtaher Safarzadeh

Although it is assumed that magnetic fields in accretion disks are dragged from the interstellar medium, the idea is likely not applicable to primordial black holes (PBHs) formed i…