activity
20152020
most citedGas flow in barred potentials

125 citations · 576 across the 10 of their papers we have counts for

collaborators

12 papers

astro-ph.GA202013 cited

Unusual Galactic HII Regions at the Intersection of the Central Molecular Zone and the Far Dust Lane

Loren D. Anderson, Mattia C. Sormani, Adam Ginsburg +7

Sgr E is a massive star formation complex found toward the Galactic center that consists of numerous discrete, compact HII regions. It is located at the intersection between the Ce…

astro-ph.GA2020

Do nuclear rings in barred galaxies form at the shear minimum of the rotation curve?

Mattia C. Sormani, Zhi Li

It has been recently suggested that (i) nuclear rings in barred galaxies (including our own Milky Way) form at the radius where the shear parameter of the rotation curve reaches a…

astro-ph.GA2019110 cited

The Cloud Factory I: Generating resolved filamentary molecular clouds from galactic-scale forces

Rowan J. Smith, Robin G. Treß, Mattia C. Sormani +6

We introduce a new suite of simulations, "The Cloud Factory", which self-consistently forms molecular cloud complexes at high enough resolution to resolve internal substructure (up…

astro-ph.GA201998 cited

Simulations of the star-forming molecular gas in an interacting M51-like galaxy

Robin G. Tress, Rowan J. Smith, Mattia C. Sormani +4

We present here the first of a series of papers aimed at better understanding the evolution and properties of giant molecular clouds (GMCs) in a galactic context. We perform high r…

astro-ph.GA2019

The geometry of the gas surrounding the Central Molecular Zone: on the origin of localised molecular clouds with extreme velocity dispersions

Mattia C. Sormani, Robin G. Tress, Simon C. O. Glover +6

Observations of molecular gas near the Galactic centre (, ) reveal the presence of a distinct population of enigmatic compact clouds which are ch…

astro-ph.GA201915 cited

The effect of rotation on the thermal instability of stratified galactic atmospheres - II. The formation of High Velocity Clouds

Mattia Sormani, Emanuele Sobacchi

Whether High Velocity Clouds (HVCs) can form by condensation of the hot () Galactic corona as a consequence of thermal instabilities has been controversial.…