131 citations · 3.2k across the 129 of their papers we have counts for
9 papers · 1 filter
Simulations of the star-forming molecular gas in an interacting M51-like galaxy: cloud population statistics
Robin G. Tress, Mattia C. Sormani, Rowan J. Smith +5
To investigate how molecular clouds react to different environmental conditions at a galactic scale, we present a catalogue of giant molecular clouds resolved down to masses of $\s…
The Cloud Factory II: Gravoturbulent Kinematics of Resolved Molecular Clouds in a Galactic Potential
Andres F. Izquierdo, Rowan J. Smith, Simon C. O. Glover +6
We present a statistical analysis of the gravoturbulent velocity fluctuations in molecular cloud complexes extracted from our "Cloud Factory" galactic-scale ISM simulation suite. F…
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…
Synthetic observations of spiral arm tracers of a simulated Milky Way analog
Stefan Reissl, Jeroen M. Stil, En Chen +16
Context: The Faraday rotation measure (RM) is often used to study the magnetic field strength and orientation within the ionized medium of the Milky Way. Observations indicate a RM…
The history of dynamics and stellar feedback revealed by the HI filamentary structure in the disk of the Milky Way
J. D. Soler, H. Beuther, J. Syed +19
We present a study of the filamentary structure in the emission from the neutral atomic hydrogen (HI) at 21 cm across velocity channels in the 40'' and 1.5-km/s resolution position…
Jeans modelling of the Milky Way's nuclear stellar disc
Mattia C. Sormani, John Magorrian, Francisco Nogueras-Lara +4
The nuclear stellar disc (NSD) is a flattened stellar structure that dominates the gravitational potential of the Milky Way at Galactocentric radii $30 \lesssim R \lesssim 300{\, \…