activity
19992026
most citedA new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: Application to magnetic field amplification by gravity-driven turbulence

301 citations · 6.3k across the 162 of their papers we have counts for

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Showing 2020Show all

10 papers · 1 filter

astro-ph.GA2020★ 34 cited

Radiation Hydrodynamical Simulations of the Birth of Intermediate-Mass Black Holes in the First Galaxies

Muhammad A. Latif, Sadegh Khochfar, Dominik Schleicher +1

The leading contenders for the seeds of quasars are direct-collapse black holes (DCBHs) forming in atomically-cooled halos at 20. However, the Lyman-Werner (LW) UV…

astro-ph.GA2020★ 43 cited

Formation of supermassive black hole seeds in nuclear star clusters via gas accretion and runaway collisions

Arpan Das, Dominik R. G. Schleicher, Nathan W. C. Leigh +1

More than two hundred supermassive black holes (SMBHs) of masses have been discovered at . One promising pathway for the formation o…

astro-ph.GA2020★ 4 cited

Small-N Collisional Dynamics V: Beyond the Realm of Not-So-Small-N

Carlos Barrera, Nathan W. C. Leigh, Bastián Reinoso +2

Direct collisions between finite-sized particles occur commonly in many areas of astrophysics. Such collisions are typically mediated by chaotic, bound gravitational interactions i…

astro-ph.GA2020★ 5 cited

Stellar Initial Mass Function over a range of redshifts

Rafeel Riaz, Dominik R. G. Schleicher, Siegfried Vanaverbeke +1

The stellar Initial Mass Function (IMF) seems to be close to universal in the local star-forming regions. However, this quantity of a newborn stellar population responds differentl…

astro-ph.GA2020

Synthetic observations of deuterated molecules in massive prestellar cores

Joaquin Zamponi F., Andrea Giannetti, Stefano Bovino +5

Young massive stars are usually found embedded in dense massive molecular clumps and are known for being highly obscured and distant. During their formation process, deuteration is…

astro-ph.GA2020★ 11 cited

Formation of Pop II star clusters in the aftermath of a pair instability supernova

Muhammad A. Latif, Dominik Schleicher

Pop II stars formed a few hundred million years after the Big Bang were key drivers of cosmic reionization and building blocks of high redshift galaxies. How and when these stars f…