activity
20172022
most citedInitial Conditions for Star Formation: A Physical Description of the Filamentary ISM

43 citations · 95 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202214 cited

Bird's eye view of molecular clouds in the Milky Way: II. Cloud kinematics from sub-pc to kpc scales

Andri Spilker, Jouni Kainulainen, Jan Orkisz

The kinematics of molecular gas are crucial for setting the stage for star formation. One key question related to the kinematic properties of gas is how they depend on the spatial…

astro-ph.GA202227 cited

3D shape explains star formation mystery of California and Orion A

Sara Rezaei Kh., Jouni Kainulainen

The new Gaia data release (EDR3) with improved astrometry has opened a new era in studying our Milky Way in fine detail. We use Gaia EDR3 astrometry together with 2MASS and WISE ph…

astro-ph.GA202243 cited

Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM

A. Hacar, S Clark, F. Heitsch +4

The interstellar medium contains filamentary structure over a wide range of scales. Understanding the role of this structure, both as a conduit of gas across the scales and a diagn…

astro-ph.GA2020

Tracers of the ionization fraction in dense and translucent gas: I. Automated exploitation of massive astrochemical model grids

Emeric Bron, Evelyne Roueff, Maryvonne Gerin +21

The ionization fraction plays a key role in the physics and chemistry of the neutral interstellar medium, from controlling the coupling of the gas to the magnetic field to allowing…

astro-ph.GA2020

C18O, 13CO, and 12CO abundances and excitation temperatures in the Orion B molecular cloud: An analysis of the precision achievable when modeling spectral line within the Local Thermodynamic Equilibrium approximation

Antoine Roueff, Maryvonne Gerin, Pierre Gratier +23

CO isotopologue transitions are routinely observed in molecular clouds to probe the column density of the gas, the elemental ratios of carbon and oxygen, and to trace the kinematic…

astro-ph.GA2019

Dynamics of cluster-forming hub-filament systems: The case of the high-mass star-forming complex Monoceros R2

S. P. Trevino-Morales, A. Fuente, A. Sanchez-Monge +15

High-mass stars and star clusters commonly form within hub-filament systems. Monoceros R2, harbors one of the closest such systems, making it an excellent target for case studies.…