What is he best known for?
The fields of study he is best known for:
- Quantum mechanics
- Astrophysics
- Astronomy
Ralf S. Klessen mainly investigates Astrophysics, Star formation, Molecular cloud, Stars and Turbulence.
His study connects Astronomy and Astrophysics.
The various areas that he examines in his Star formation study include Gravitational collapse, Metallicity and Stellar evolution.
His Molecular cloud research integrates issues from Mass spectrum, Line, Magnetohydrodynamics, Spectral line and Radiative transfer.
The concepts of his Stars study are interwoven with issues in Mass distribution, Physical cosmology, Magnetic field and Halo.
His Turbulence research is multidisciplinary, incorporating perspectives in Solenoidal vector field, Mach number, Power law and Supersonic speed.
His most cited work include:
- Control of star formation by supersonic turbulence (1436 citations)
- Comparing the statistics of interstellar turbulence in simulations and observations - Solenoidal versus compressive turbulence forcing (687 citations)
- The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations (525 citations)
What are the main themes of his work throughout his whole career to date?
Astrophysics, Star formation, Molecular cloud, Stars and Astronomy are his primary areas of study.
His Astrophysics study frequently draws connections to other fields, such as Turbulence.
His Turbulence research is multidisciplinary, relying on both Computational physics, Supersonic speed, Magnetic field and Mach number.
His Star formation study combines topics in areas such as Gravitational collapse, Metallicity and Star cluster.
His research integrates issues of Line, Magnetohydrodynamics, Power law, Gravitation and Radiative transfer in his study of Molecular cloud.
His Stars study incorporates themes from Halo, Supernova, Dark matter and Cluster.
He most often published in these fields:
- Astrophysics (101.77%)
- Star formation (59.36%)
- Molecular cloud (43.23%)
What were the highlights of his more recent work (between 2017-2021)?
- Astrophysics (101.77%)
- Star formation (59.36%)
- Stars (43.35%)
In recent papers he was focusing on the following fields of study:
His primary areas of study are Astrophysics, Star formation, Stars, Galaxy and Molecular cloud.
His work in Interstellar medium, Milky Way, Star cluster, Line and Spiral galaxy is related to Astrophysics.
Within one scientific family, Ralf S. Klessen focuses on topics pertaining to Stellar dynamics under Star formation, and may sometimes address concerns connected to Boundary.
His study focuses on the intersection of Stars and fields such as Halo with connections in the field of Dark matter.
Ralf S. Klessen has included themes like Gravitation, Radiative transfer, Radiation pressure and Velocity dispersion in his Molecular cloud study.
Ralf S. Klessen focuses mostly in the field of Radiative transfer, narrowing it down to matters related to Computational physics and, in some cases, Turbulence.
Between 2017 and 2021, his most popular works were:
- Analyzing Inverse Problems with Invertible Neural Networks (94 citations)
- The evolution of supermassive Population III stars (70 citations)
- A theoretical explanation for the Central Molecular Zone asymmetry (55 citations)
In his most recent research, the most cited papers focused on:
- Quantum mechanics
- Galaxy
- Astrophysics
Ralf S. Klessen focuses on Astrophysics, Star formation, Stars, Galaxy and Molecular cloud.
Ralf S. Klessen combines topics linked to Spectral line with his work on Astrophysics.
His work carried out in the field of Star formation brings together such families of science as Line and Redshift, Reionization.
Ralf S. Klessen has researched Stars in several fields, including Dark Ages and Cluster.
His Molecular cloud study combines topics from a wide range of disciplines, such as Large Magellanic Cloud, Nebula, Substructure, Line-of-sight and Radiative transfer.
His study looks at the intersection of Star cluster and topics like Solar mass with Gravitation and Initial mass function.
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