activity
20192022
most citedA dynamically young, gravitationally stable network of filaments in Orion B

37 citations · 109 across the 5 of their papers we have counts for

collaborators

9 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.GA202127 cited

Bird's eye view of molecular clouds in the Milky Way: I. Column density and star formation from sub-pc to kpc scales

Andri Spilker, Jouni Kainulainen, Jan Orkisz

Describing how the properties of the interstellar medium combine across size-scales is crucial for understanding star formation scaling laws and connecting Galactic and extragalact…

astro-ph.GA2020

Quantitative inference of the column densities from 3 mm molecular emission: A case study towards Orion B

Pierre Gratier, Jérôme Pety, Emeric Bron +21

Molecular hydrogen being unobservable in cold molecular clouds, the column density measurements of molecular gas currently rely either on dust emission observation in the far-IR or…

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.GA20204 cited

Autonomous Gaussian decomposition of the Galactic Ring Survey. II. The Galactic distribution of 13CO

M. Riener, J. Kainulainen, J. D. Henshaw +1

Knowledge about the distribution of CO emission in the Milky Way is essential to understand the impact of Galactic environment on the formation and evolution of structures in the i…

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…