Jouni Kainulainen
Jouni Kainulainen’s research focuses on how new stars are born in the Milky Way and what is the life-cycle of the interstellar medium. The goal of his research is to understand the physical processes that determine where, when, and how new stars form in galaxies like the one we live in.
Jouni Kainulainen leads an ERC-grant supported research group that addresses these questions with the help of both observational data and theoretical work.
Showing 37 publications
Deep learning denoising by dimension reduction: Application to the ORION-B line cubes
Initial Conditions for Star Formation: a Physical Description of the Filamentary ISM
Gas kinematics around filamentary structures in the Orion B cloud
The width of Herschel filaments varies with distance
The effect of viewing angle on the Kennicutt-Schmidt relation of the local molecular clouds
Dust extinction map of the Galactic plane based on the VVV survey data
Three-dimensional Shape Explains Star Formation Mystery of California and Orion A
The SEDIGISM survey: Molecular clouds in the inner Galaxy
SEDIGISM-ATLASGAL: Dense gas fraction and star formation efficiency across the Galactic disc
The SEDIGISM survey: First Data Release and overview of the Galactic structure
Ubiquitous velocity fluctuations throughout the molecular interstellar medium
Autonomous Gaussian decomposition of the Galactic Ring Survey: II. The Galactic distribution of 13CO
Star-forming content of the giant molecular filaments in the Milky Way
Deep point spread function photometric catalog of the VVV survey data
GAUSSPY+: A fully automated Gaussian decomposition package for emission line spectra
Histogram of oriented gradients: a technique for the study of molecular cloud formation
OH maser emission in the THOR survey of the northern Milky Way
SEDIGISM: the kinematics of ATLASGAL filaments
Structure and fragmentation of a high line-mass filament: Nessie
The Stellar Content of the Infalling Molecular Clump G286.21+0.17
Prestellar and protostellar cores in Orion B9
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Showing 3 research projects
The Bird's Eye Milky Way: Gaias syn på täthetsdiagnostiken för stjärnbildning
Turbulensdiagnostik i molekylmolnen i solens närhet
PROMISE Origins of the Molecular Cloud Structure