The compressed tarballs in this repository contain the binary output data from the SPMHD (smoothed particle magnetohydrodynamics) simulation presented in the paper. The data is a Fortran binary file in big-endian format. The DAT???? files are dumps of the simulation spaced every 1/100 of a free-fall time and can be read in Splash (Written by Daniel Price, see http://users.monash.edu.au/~dprice/splash/). The Atest_? and Ptest_? files contain information on accreted particles and sink particles respectively (again in big-endian format). The two Fortran programs in utils.tar.xz can read these files and output ASCII data. The tarballs themselves are named according to the following scheme: theta_*.tar.xz are the 1.5 million particle simulation...
This is the data created for Wurster & Bate (2019): Disc formation and fragmentation using radiative...
We numerically model the collapse of magnetic rotating protostellar clouds with mass of 10 M The sim...
This is the final version. Available from Frontiers Media via the DOI in this record. The formation ...
The dataset used to produce this paper can be accessed at http://hdl.handle.net/10871/17109 Animati...
The compressed tarballs in this repository contain the binary output data from the SPMHD (smoothed p...
Published onlineThis is the final version of the article. Available from Oxford University Press via...
The properties which define a molecular cloud core — the evolutionary phase bridging between a molec...
The compressed tarballs in this repository contain the binary output data from the SPMHD (smoothed p...
The XZ compressed tarballs in this repository contain the binary output data from the smoothed parti...
Magnetic fields are known to play a crucial role in the star formation process, particularly in the ...
This is the data created for Wurster, Bate & Price (2018c): Hall effect-driven formation of gravitat...
The protostellar collapse of a molecular cloud core is usually accompanied by outflow phenomena. The...
This is all the data created for Wurster, Bate & Price (2018a). This dataset was created using the ...
This repository contains the datasets from the original smoothed particle hydrodynamics (SPH) calcul...
This is the final published version, also available from Oxford University Press via the DOI in this...
This is the data created for Wurster & Bate (2019): Disc formation and fragmentation using radiative...
We numerically model the collapse of magnetic rotating protostellar clouds with mass of 10 M The sim...
This is the final version. Available from Frontiers Media via the DOI in this record. The formation ...
The dataset used to produce this paper can be accessed at http://hdl.handle.net/10871/17109 Animati...
The compressed tarballs in this repository contain the binary output data from the SPMHD (smoothed p...
Published onlineThis is the final version of the article. Available from Oxford University Press via...
The properties which define a molecular cloud core — the evolutionary phase bridging between a molec...
The compressed tarballs in this repository contain the binary output data from the SPMHD (smoothed p...
The XZ compressed tarballs in this repository contain the binary output data from the smoothed parti...
Magnetic fields are known to play a crucial role in the star formation process, particularly in the ...
This is the data created for Wurster, Bate & Price (2018c): Hall effect-driven formation of gravitat...
The protostellar collapse of a molecular cloud core is usually accompanied by outflow phenomena. The...
This is all the data created for Wurster, Bate & Price (2018a). This dataset was created using the ...
This repository contains the datasets from the original smoothed particle hydrodynamics (SPH) calcul...
This is the final published version, also available from Oxford University Press via the DOI in this...
This is the data created for Wurster & Bate (2019): Disc formation and fragmentation using radiative...
We numerically model the collapse of magnetic rotating protostellar clouds with mass of 10 M The sim...
This is the final version. Available from Frontiers Media via the DOI in this record. The formation ...