Lista de obras - Jouni Kainulainen - Dominio Público Uruguay

A comparison of density structures of a star forming and a non-star-forming globule DCld 303.8-14.2 and Thumbprint Nebula

artículo científico publicado en 2007

A transient Sub-Eddington black hole X-ray binary candidate in the dust lanes of Centaurus A ⬇️

artículo científico publicado en 2012

A virialized filamentary infrared dark cloud ⬇️

scholarly article

Appearance of dusty filaments at different viewing angles ⬇️

artículo científico publicado en 2016

C 18 O, 13 CO, and 12 CO abundances and excitation temperatures in the Orion B molecular cloud

Connection between dense gas mass fraction, turbulence driving, and star formation efficiency of molecular clouds

scholarly article

Constraining the Dust Opacity Law in Three Small and Isolated Molecular Clouds

scientific article published in the Astrophysical Journal

Deep point spread function photometric catalog of the VVV survey data

artículo científico publicado en 2019

Dense cores in the Pipe Nebula: an improved core mass function ⬇️

artículo científico publicado en 2009

Determination of the mass function of extra-galactic GMCs via NIR color maps. Testing the method in a disk-like geometry

artículo científico publicado en 2007

Dust-temperature of an isolated star-forming cloud:Herschelobservations of the Bok globule CB244

scientific article published in Astronomy and Astrophysics

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

scientific article published on 12 September 2019

Earliest phases of star formation (EPoS) Dust temperature distributions in isolated starless cores ⬇️

artículo científico publicado en 2016

Error Propagation in Calibration Networks of Synthetic Aperture Radiometers

Evolution of column density distributions within Orion A ⬇️

artículo científico publicado en 2015

GAUSSPY+: A fully automated Gaussian decomposition package for emission line spectra

scholarly article

Gas kinematics and excitation in the filamentary IRDC G035.39-00.33 ⬇️

artículo científico publicado en 2014

Giant molecular filaments in the Milky Way ⬇️

artículo científico publicado en 2016

Giant molecular filaments in the Milky Way ⬇️

artículo científico publicado en 2014

Gravitational fragmentation caught in the act: the filamentary Musca molecular cloud ⬇️

artículo científico publicado en 2016

Helical magnetic fields in molecular clouds? - A new method to determine the line-of-sight magnetic field structure in molecular clouds

artículo científico publicado en 2018

Helsinki University of Technology L-Band Airborne Synthetic Aperture Radiometer

article published in 2008

High-dynamic-range extinction mapping of infrared dark clouds. Dependence of density variance with sonic mach number in molecular clouds

artículo científico publicado en 2013

High-fidelity view of the structure and fragmentation of the high-mass, filamentary IRDC G11.11-0.12

artículo científico publicado en 2013

Histogram of oriented gradients: a technique for the study of molecular cloud formation

scholarly article

Mass reservoirs surrounding massive infrared dark clouds. A view by near-infrared dust extinction

artículo científico publicado en 2011

Near-infrared reddening of extra-galactic giant molecular clouds in a face-on geometry

artículo científico publicado en 2008

OH absorption in the first quadrant of the Milky Way as seen by THOR

artículo científico publicado en 2018

On the fragmentation of filaments in a molecular cloud simulation

artículo científico publicado en 2018

Opacity broadening of ^13^CO linewidths and its effect on the variance-sonic mach number relation ⬇️

artículo científico publicado en 2014

Prestellar and protostellar cores in Orion B9

artículo científico publicado en 2009

Probing the evolution of molecular cloud structure. From quiescence to birth

artículo científico publicado en 2009

Probing the evolution of molecular cloud structure. II. From chaos to confinement

scholarly article

Protostars and stars in the coronet cluster: age, evolution, and cluster structure ⬇️

Quantitative inference of the H 2 column densities from 3 mm molecular emission: case study towards Orion B

Radio brightness validation on different spatial scales during the SMOS validation campaign 2010 in the Rur catchment, Germany

article

Relationship between the column density distribution and evolutionary class of molecular clouds as viewed by ATLASGAL ⬇️

artículo científico publicado en 2015

Relationship between turbulence energy and density variance in the solar neighbourhood molecular clouds

scholarly article

Resolving the fragmentation of high line-mass filaments with ALMA: the integral shaped filament in Orion A ⬇️

scientific article published in Astronomy and Astrophysics

Revealing which Combinations of Molecular Lines are Sensitive to the Gas Physical Parameters of Molecular Clouds

artículo científico publicado en 2022

SEDIGISM-ATLASGAL: dense gas fraction and star formation efficiency across the Galactic disc

artículo científico publicado en 2020

SEDIGISM: the kinematics of ATLASGAL filaments

artículo científico publicado en 2018

SMOS Calibration Subsystem

SMOS instrument performance and calibration after six years in orbit

scholarly article by M. Martín-Neira et al published July 2016 in Remote Sensing of Environment

Sequential star formation in IRAS 06084-0611 (GGD 12-15). From intermediate-mass to high-mass stars

artículo científico publicado en 2011

Smos payload performance assessment

Spectral properties of X-ray binaries in Centaurus A ⬇️

artículo científico publicado en 2013

Star formation in the Taurus filament L 1495: from dense cores to stars ⬇️

artículo científico publicado en 2010

Star-forming content of the giant molecular filaments in the Milky Way

artículo científico publicado en 2019

Structure and fragmentation of a high line-mass filament: Nessie

artículo científico publicado en 2018

The Arizona Radio Observatory CO Mapping Survey of Galactic Molecular Clouds. VI. The Cep OB3 Cloud (Cepheus B and C) in CO J = 2–1, 13CO J = 2–1, and CO J = 3–2

The Coalsack near and far

artículo científico publicado en 2011

The Earliest Phases of Star Formation (EPoS): a Herschel key project. The thermal structure of low-mass molecular cloud cores

artículo científico publicado en 2013

The Earliest Phases of Star formation (EPoS) observed withHerschel: the dust temperature and density distributions of B68

scientific article published in Astronomy and Astrophysics

The HI/OH/Recombination line survey of the inner Milky Way (THOR) ⬇️

artículo científico publicado en 2016

The Musca cloud: A 6 pc-long velocity-coherent, sonic filament ⬇️

scientific article published in Astronomy and Astrophysics

The SEDIGISM survey: First Data Release and overview of the Galactic structure

artículo científico publicado en 2020

The SEDIGISM survey: molecular clouds in the inner Galaxy

artículo científico publicado en 2020

The Star Formation in the L1615/L1616 Cometary Cloud ⬇️

artículo científico publicado en 2008

The darkest shadows: deep mid-infrared extinction mapping of a massive protocluster ⬇️

artículo científico publicado en 2014

The distribution of mass surface densities in a high-mass protocluster ⬇️

artículo científico publicado en 2016

The effect of viewing angle on the Kennicutt-Schmidt relation of the local molecular clouds

artículo científico publicado en 2022

The fidelity of the core mass functions derived from dust column density data

artículo científico publicado en 2009

The link between magnetic fields and filamentary clouds: bimodal cloud orientations in the Gould Belt

scholarly article

The optical-infrared extinction curve and its variation in the Milky Way ⬇️

artículo científico publicado en 2016

The ratio of N(C^18^O) and A_V_ in Chamaeleon I and III-B. Using 2MASS and SEST

artículo científico publicado en 2006

The stellar content of the infalling molecular clump G286.21+0.17 ⬇️

artículo científico publicado en 2017

Tracers of the ionization fraction in dense and translucent gas

Unfolding the Laws of Star Formation: The Density Distribution of Molecular Clouds

artículo científico publicado en 2014

VISION − Vienna survey in Orion ⬇️

scientific article published in Astronomy and Astrophysics

Young massive star cluster formation in the Galactic Centre is driven by global gravitational collapse of high-mass molecular clouds

artículo científico publicado en 2019

Lista de obras de Jouni Kainulainen

A comparison of density structures of a star forming and a non-star-forming globule DCld 303.8-14.2 and Thumbprint Nebula

A transient Sub-Eddington black hole X-ray binary candidate in the dust lanes of Centaurus A ⬇️

A virialized filamentary infrared dark cloud ⬇️

Appearance of dusty filaments at different viewing angles ⬇️

C 18 O, 13 CO, and 12 CO abundances and excitation temperatures in the Orion B molecular cloud

Connection between dense gas mass fraction, turbulence driving, and star formation efficiency of molecular clouds

Constraining the Dust Opacity Law in Three Small and Isolated Molecular Clouds

Deep point spread function photometric catalog of the VVV survey data

Dense cores in the Pipe Nebula: an improved core mass function ⬇️

Determination of the mass function of extra-galactic GMCs via NIR color maps. Testing the method in a disk-like geometry

Dust-temperature of an isolated star-forming cloud:Herschelobservations of the Bok globule CB244

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

Earliest phases of star formation (EPoS) Dust temperature distributions in isolated starless cores ⬇️

Error Propagation in Calibration Networks of Synthetic Aperture Radiometers

Evolution of column density distributions within Orion A ⬇️

GAUSSPY+: A fully automated Gaussian decomposition package for emission line spectra

Gas kinematics and excitation in the filamentary IRDC G035.39-00.33 ⬇️

Giant molecular filaments in the Milky Way ⬇️

Giant molecular filaments in the Milky Way ⬇️

Gravitational fragmentation caught in the act: the filamentary Musca molecular cloud ⬇️

Helical magnetic fields in molecular clouds? - A new method to determine the line-of-sight magnetic field structure in molecular clouds

Helsinki University of Technology L-Band Airborne Synthetic Aperture Radiometer

High-dynamic-range extinction mapping of infrared dark clouds. Dependence of density variance with sonic mach number in molecular clouds

High-fidelity view of the structure and fragmentation of the high-mass, filamentary IRDC G11.11-0.12

Histogram of oriented gradients: a technique for the study of molecular cloud formation

Mass reservoirs surrounding massive infrared dark clouds. A view by near-infrared dust extinction

Near-infrared reddening of extra-galactic giant molecular clouds in a face-on geometry

OH absorption in the first quadrant of the Milky Way as seen by THOR

On the fragmentation of filaments in a molecular cloud simulation

Opacity broadening of ^13^CO linewidths and its effect on the variance-sonic mach number relation ⬇️

Prestellar and protostellar cores in Orion B9

Probing the evolution of molecular cloud structure. From quiescence to birth

Probing the evolution of molecular cloud structure. II. From chaos to confinement

Protostars and stars in the coronet cluster: age, evolution, and cluster structure ⬇️

Quantitative inference of the H 2 column densities from 3 mm molecular emission: case study towards Orion B

Radio brightness validation on different spatial scales during the SMOS validation campaign 2010 in the Rur catchment, Germany

Relationship between the column density distribution and evolutionary class of molecular clouds as viewed by ATLASGAL ⬇️

Relationship between turbulence energy and density variance in the solar neighbourhood molecular clouds

Resolving the fragmentation of high line-mass filaments with ALMA: the integral shaped filament in Orion A ⬇️

Revealing which Combinations of Molecular Lines are Sensitive to the Gas Physical Parameters of Molecular Clouds

SEDIGISM-ATLASGAL: dense gas fraction and star formation efficiency across the Galactic disc

SEDIGISM: the kinematics of ATLASGAL filaments

SMOS Calibration Subsystem

SMOS instrument performance and calibration after six years in orbit

Sequential star formation in IRAS 06084-0611 (GGD 12-15). From intermediate-mass to high-mass stars

Smos payload performance assessment

Spectral properties of X-ray binaries in Centaurus A ⬇️

Star formation in the Taurus filament L 1495: from dense cores to stars ⬇️

Star-forming content of the giant molecular filaments in the Milky Way

Structure and fragmentation of a high line-mass filament: Nessie

The Arizona Radio Observatory CO Mapping Survey of Galactic Molecular Clouds. VI. The Cep OB3 Cloud (Cepheus B and C) in CO J = 2–1, 13CO J = 2–1, and CO J = 3–2

The Coalsack near and far

The Earliest Phases of Star Formation (EPoS): a Herschel key project. The thermal structure of low-mass molecular cloud cores

The Earliest Phases of Star formation (EPoS) observed withHerschel: the dust temperature and density distributions of B68

The HI/OH/Recombination line survey of the inner Milky Way (THOR) ⬇️

The Musca cloud: A 6 pc-long velocity-coherent, sonic filament ⬇️

The SEDIGISM survey: First Data Release and overview of the Galactic structure

The SEDIGISM survey: molecular clouds in the inner Galaxy

The Star Formation in the L1615/L1616 Cometary Cloud ⬇️

The darkest shadows: deep mid-infrared extinction mapping of a massive protocluster ⬇️

The distribution of mass surface densities in a high-mass protocluster ⬇️

The effect of viewing angle on the Kennicutt-Schmidt relation of the local molecular clouds

The fidelity of the core mass functions derived from dust column density data

The link between magnetic fields and filamentary clouds: bimodal cloud orientations in the Gould Belt

The optical-infrared extinction curve and its variation in the Milky Way ⬇️

The ratio of N(C^18^O) and A_V_ in Chamaeleon I and III-B. Using 2MASS and SEST

The stellar content of the infalling molecular clump G286.21+0.17 ⬇️

Tracers of the ionization fraction in dense and translucent gas

Unfolding the Laws of Star Formation: The Density Distribution of Molecular Clouds

VISION − Vienna survey in Orion ⬇️

Young massive star cluster formation in the Galactic Centre is driven by global gravitational collapse of high-mass molecular clouds