Jove
Visualize
Contact Us
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Filters

Christoph Federrath

Showing results (1-10 of 8) with videos related to

Pageof 1
Sort By:
Science (New York, N.Y.)|April 12, 2014
Unfolding the laws of star formation: the density distribution of molecular cloudsJouni Kainulainen, Christoph Federrath, Thomas Henning
Physical Review Letters|December 31, 2008
Is the scaling of supersonic turbulence universal?Wolfram Schmidt, Christoph Federrath, Ralf Klessen
Monthly Notices of the Royal Astronomical Society|October 7, 2022
Environmental variation of the low-mass IMFTabassum S Tanvir, Mark R Krumholz, Christoph Federrath
Monthly Notices of the Royal Astronomical Society|October 25, 2024
AHKASH: a new Hybrid particle-in-cell code for simulations of astrophysical collisionless plasmaRadhika Achikanath Chirakkara, Christoph Federrath, Amit Seta
Physical Review Letters|March 22, 2021
Efficient Highly Subsonic Turbulent Dynamo and Growth of Primordial Magnetic FieldsRadhika Achikanath Chirakkara, Christoph Federrath, Pranjal Trivedi, et al.
Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics|April 3, 2012
Magnetic field amplification by small-scale dynamo action: dependence on turbulence models and Reynolds and Prandtl numbersJennifer Schober, Dominik Schleicher, Christoph Federrath, et al.
Monthly Notices of the Royal Astronomical Society|March 30, 2021
Magnetic field amplification in accretion discs around the first stars: implications for the primordial IMFPiyush Sharda, Christoph Federrath, Mark R Krumholz, et al.
Physical Review. E|July 20, 2022
Turbulence generation by shock interaction with a highly nonuniform mediumSeth Davidovits, Christoph Federrath, Romain Teyssier, et al.
Pageof 1

Showing results (1-10 of 8) with videos related to

Sort By:
Pageof 1
Science (New York, N.Y.)|April 12, 2014
Unfolding the laws of star formation: the density distribution of molecular cloudsJouni Kainulainen, Christoph Federrath, Thomas Henning
Physical Review Letters|December 31, 2008
Is the scaling of supersonic turbulence universal?Wolfram Schmidt, Christoph Federrath, Ralf Klessen
Monthly Notices of the Royal Astronomical Society|October 7, 2022
Environmental variation of the low-mass IMFTabassum S Tanvir, Mark R Krumholz, Christoph Federrath
Monthly Notices of the Royal Astronomical Society|October 25, 2024
AHKASH: a new Hybrid particle-in-cell code for simulations of astrophysical collisionless plasmaRadhika Achikanath Chirakkara, Christoph Federrath, Amit Seta
Physical Review Letters|March 22, 2021
Efficient Highly Subsonic Turbulent Dynamo and Growth of Primordial Magnetic FieldsRadhika Achikanath Chirakkara, Christoph Federrath, Pranjal Trivedi, et al.
Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics|April 3, 2012
Magnetic field amplification by small-scale dynamo action: dependence on turbulence models and Reynolds and Prandtl numbersJennifer Schober, Dominik Schleicher, Christoph Federrath, et al.
Monthly Notices of the Royal Astronomical Society|March 30, 2021
Magnetic field amplification in accretion discs around the first stars: implications for the primordial IMFPiyush Sharda, Christoph Federrath, Mark R Krumholz, et al.
Physical Review. E|July 20, 2022
Turbulence generation by shock interaction with a highly nonuniform mediumSeth Davidovits, Christoph Federrath, Romain Teyssier, et al.
Pageof 1