Ralf Klessen
Klessen, Ralf S., 1968-
![Sudoc [ABES], France](/viaf/images/flags/SUDOC.png "Sudoc [ABES], France")
Klessen, Ralf S.
Klessen, Ralf 1968-....
VIAF ID: 62381423 (Personal)
Permalink: http://viaf.org/viaf/62381423
Preferred Forms
-
200 _ |
‡a
Klessen
‡b
Ralf
‡f
1968-....
-
100 1 _ ‡a Klessen, Ralf S.
-
100 1 _
‡a
Klessen, Ralf S.
-
100 1 _ ‡a Klessen, Ralf S.
-
100 1 _ ‡a Klessen, Ralf S. (sparse)
-
100 1 _
‡a
Klessen, Ralf S.
‡d
1968-
-
100 1 _
‡a
Klessen, Ralf S.,
‡d
1968-
-
100 0 _
‡a
Ralf Klessen
-
100 0 _
‡a
Ralf Klessen
4xx's: Alternate Name Forms (14)
5xx's: Related Names (5)
- 551 _ _
‡a
Erlangen
‡4
ortg
‡4
https://d-nb.info/standards/elementset/gnd#placeOfBirth
- 551 _ _
‡a
Heidelberg
‡4
ortw
‡4
https://d-nb.info/standards/elementset/gnd#placeOfActivity
- 510 2 _
‡a
Potsdam, Univ
- 510 2 _
‡a
Zentrum für Astronomie
‡g
Heidelberg
‡4
affi
‡4
https://d-nb.info/standards/elementset/gnd#affiliation
‡e
Affiliation
- 510 2 _
‡a
Zentrum für Astronomie (Heidelberg)
Works
| Title | Sources |
|---|---|
| Characterising Pre-Main-Sequence Stars in the Large Magellanic Cloud with Machine and Deep Learning Techniques |
|
| Comparison of Different Star Formation Tracers in Nearby AGN Host Galaxies |
|
| Cosmological Transition to Metal-Enriched Star-Formation |
|
| Delaying the formation of the first stars The impact of streaming velocities and Lyman-Werner radiation in cosmological hydrodynamical simulations |
|
| Embedded star clusters surviving gas expulsion with low star formation efficiencies. |
|
| Formation and growth of the first supermassive black holes |
|
| La formation du gaz dense à l'origine des étoiles de faible et de haute masse |
|
| Formation et croissance des premiers trous noirs supermassifs. |
|
| The formation of dense gas in low- and high-mass star forming regions. |
|
| Formation of massive black hole seeds through runaway stellar collisions and gas accretion in dense stellar systems |
|
| Fragmentation of molecular clouds the initial phases of a stellar cluster |
|
| From galactic dynamics to star formation, what sets the star formation rate?. |
|
| The HI/OH/Recombination line survey of the inner Milky Way (THOR) |
|
| Hierarchical stellar structures in the Local Group dwarf galaxy NGC 6822 |
|
| A holistic scenario of turbulent molecular cloud evolution and control of the star formation efficiency: first tests |
|
| Impact of supernova and cosmic-ray driving on the surface brightness of the galactic halo in soft x-rays |
|
| The impact of thermodynamics on gravitational collapse: filament formation and magnetic field amplification |
|
| Importance of the initial conditions for star formation - III. Statistical properties of embedded protostellar clusters |
|
| The interplay of magnetic fields, fragmentation, and ionization feedback in high-mass star formation |
|
| ISM dynamics in simulated galaxies: bridging the scales |
|
| Kinetic Energy Decay Rates of Supersonic and Super-Alfvénic Turbulence in Star-Forming Clouds |
|
| De la dynamique galactique à la formation stellaire : comment est régulé le taux de formation d'étoiles ? |
|
| Line profiles of cores within clusters. II. Signatures of dynamical collapse during high-mass star formation |
|
| The link between molecular cloud structure and turbulence |
|
| Mach Number Dependence of Turbulent Magnetic Field Amplification: Solenoidal versus Compressive Flows |
|
| The mass spectra of cores in turbulent molecular clouds and implications for the initial mass function |
|
| The mean surface density of companions in a stellar-dynamical context |
|
| Metallicity evolution of direct collapse black hole hosts: CR7 as a case study |
|
| Modeling dust evolution in galaxies with a multiphase, inhomogeneous ISM |
|
| Molecular cloud evolution. II. From cloud formation to the early stages of star formation in decaying conditions |
|
| A multishock model for the density variance of anisotropic, highly magnetized, supersonic turbulence |
|
| A new jeans resolution criterion for (M)HD simulations of self-gravitating gas: application to magnetic field amplification by gravity-driven turbulence |
|
| Number ratios of young stellar objects in embedded clusters |
|
| Numerical and semi-analytic core mass distributions in supersonic isothermal turbulence |
|
| On the evolution of the density probability density function in strongly self-gravitating systems |
|
| On the structure of self-gravitating molecular clouds |
|
| On the temperature structure of the galactic center cloud G0.253+0.016 |
|
| The origin of dust polarization in molecular outflows |
|
| PHANGS–ALMA: Arcsecond CO(2–1) Imaging of Nearby Star-forming Galaxies |
|
| The PHANGS-HST Survey: Physics at High Angular Resolution in Nearby Galaxies with the Hubble Space Telescope |
|
| Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies |
|
| Probing high-redshift quasars with ALMA. I. Expected observables and potential number of sources |
|
| Protostars and planets VI |
|
| relation between interstellar turbulence and star formation |
|
| The reliability of approximate radiation transport methods for irradiated disk studies |
|
| The reliability of observational measurements of column density probability distribution functions |
|
| Saturation of the turbulent dynamo. |
|
| Secret Lives of Young Massive Star Clusters |
|
| Simulations of the star-forming molecular gas in an interacting M51-like galaxy: cloud population statistics |
|
| Simulations on a moving mesh: the clustered formation of population III protostars |
|
| The small-scale dynamo and non-ideal magnetohydrodynamics in primordial star formation |
|
| Small-scale dynamo at low magnetic Prandtl numbers. |
|
| Spectral shifting strongly constrains molecular cloud disruption by radiation pressure on dust |
|
| Star formation at very low metallicity. II. On the insignificance of metal-line cooling during the early stages of gravitational collapse |
|
| Star formation at very low metallicity. V. The greater importance of initial conditions compared to metallicity thresholds |
|
| Star Formation in Galaxy Evolution: Connecting Numerical Models to Reality Saas-Fee Advanced Course 43. Swiss Society for Astrophysics and Astronomy |
|
| Star formation in isolated disk galaxies. II. Schmidt laws and efficiency of gravitational collapse |
|
| The star formation rate of turbulent magnetized clouds: comparing theory, simulations, and observations |
|
| Stars and star formation in the Milky Way system |
|
| Statistical properties of dark matter mini-haloes at z ≥ 15 |
|
| Statistical properties of supersonic turbulence in the Lagrangian and Eulerian frameworks |
|
| The stellar mass spectrum from non-isothermal gravoturbulent fragmentation |
|
| Sternentstehung vom Urknall bis zur Geburt der Sonne |
|
| TOPoS. I. Survey design and analysis of the first sample |
|
| TOPoS. II. On the bimodality of carbon abundance in CEMP stars. Implications on the early chemical evolution of galaxies |
|
| TOPoS. III. An ultra iron-poor multiple CEMP system |
|
| TOPoS. IV. Chemical abundances from high-resolution observations of seven extremely metal-poor stars |
|
| The turbulence spectrum of molecular clouds in the galactic ring survey: a density-dependent principal component analysis calibration |
|
| Turbulent mixing in the interstellar medium: an application for Lagrangian tracer particles |
|
| Ultraviolet escape fractions from giant molecular clouds during early cluster formation |
|
| Understanding spatial and spectral morphologies of ultracompact H II regions |
|
| Understanding star formation in molecular clouds. III. Probability distribution functions of molecular lines in Cygnus X |
|
| Understanding the Era of Reionization via Numerical Methods for Radiative Transfer |
|
| Weakly interacting massive particle dark matter and first stars: suppression of fragmentation in primordial star formation |
|
| Wie entstehen Sterne? |
|
