| dc.contributor.author | Lewis, Benjamin T. | |
| dc.contributor.author | Bate, Matthew R. | |
| dc.contributor.author | Price, Daniel J. | |
| dc.date.accessioned | 2016-12-07T10:42:35Z | |
| dc.date.issued | 2016-11-28 | |
| dc.date.updated | 2016-11-30T00:47:17Z | |
| dc.description.abstract | This is the dataset that was used to produce the Erratum and Addendum published in MNRAS. Included are the binary dump files from all four of the calculations in the Addendum. | en_GB |
| dc.description.sponsorship | Australian Research Council Discovery Project Grant | en_GB |
| dc.description.sponsorship | European Research Council | en_GB |
| dc.description.sponsorship | Science and Technology Facilities Council | en_GB |
| dc.description.sponsorship | University of Exeter Supercomputer: jointly funded by Science and Technology Facilities Council (STFC), Large Facilities Capital Fund of BIS, and the University of Exeter | en_GB |
| dc.description.sponsorship | DiRAC Complexity system, operated by the University of Leicester IT Services, which forms part of the STFC DiRAC HPC Facility (www.dirac.ac.uk). DiRAC is part of the National E-Infrastructure. | en_GB |
| dc.identifier.uri | http://hdl.handle.net/10871/24758 | |
| dc.language.iso | en | en_GB |
| dc.publisher | University of Exeter (dataset) / Oxford University Press (paper) | en_GB |
| dc.rights | Available under a CC-BY (v. 2.0 UK: England and Wales) License. Please acknowledge source by citing the published MNRAS paper and the ORE handle for this dataset. | en_GB |
| dc.title | Erratum and Addendum: Smoothed particle magnetohydrodynamic simulations of protostellar outflows with misaligned magnetic field and rotation axes (dataset) | en_GB |
| dc.type | Dataset | en_GB |
| dc.date.available | 2016-12-07T10:42:35Z | |
| dc.description | 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 Addendum compares the results of two calculations from the original paper (2015_0.tar.xz and 2015_45.tar.xz) with calculations performed using an SPMHD code with the integrator bug corrected (2016_0.tar.xz and 2016_45.tar.xz). | en_GB |
| dc.identifier.journal | Monthly Notices of the Royal Astronomical Society | en_GB |
