Simulation data + processed quantities for the isolated and wind cases of the Large Magellanic Cloud

We used the GIZMO-MHD code to create a simulation of the Large Magellanic Cloud with two scenarios - an isolated galaxy and a galaxy passing through the circumgalactic medium of the Milky Way and experiencing ram pressure stripping as a result of the Milky Way wind. Our mass resolution is 250 solar masses (for the medhighres cases), which is one of the best out there for galaxy simulations containing magnetic fields. While the entire simulation runs over 500 Myr astrophysical timescales, we only upload the final snapshot from both scenarios as they should be equivalent to the present-day LMC. We upload processed quantities, which account for varied radiation background at different places in the interstellar medium, and tools to calculate mock quantities like rotation measures. We also attach one snapshot + processed quantities at low resolution (called medres) for testing.
Type
collection
Title
Simulation data + processed quantities for the isolated and wind cases of the Large Magellanic Cloud
Brief Title
LMC simulation data
Alternate Title
snapshot_100 + snapshot_100_processed_quantities
Collection Type
Dataset
Access Privileges
Research School of Astronomy and Astrophysics (RSAA)
DOI - Digital Object Identifier
https://doi.org/10.1093/mnras/staf1003
Metadata Language
English
Data Language
English
Significance Statement
This is the first simulation of a dwarf galaxy called the Large Magellanic Cloud that includes magnetic fields. The work has been accepted in a prestigious journal, Monthly Notices of the Royal Astronomical Society. All the authors of this paper are from the Research School of Astronomy and Astrophysics, ANU.
Brief Description
Two snapshots + corresponding processed quantities of the simulation of LMC - isolated case and wind case at high resolution (medhighres in snapshot name). One snapshot + corresponding processed quantities of the LMC simulation at low resolution (called medres) for testing.
Full Description
We used the GIZMO-MHD code to create a simulation of the Large Magellanic Cloud with two scenarios - an isolated galaxy and a galaxy passing through the circumgalactic medium of the Milky Way and experiencing ram pressure stripping as a result of the Milky Way wind. Our mass resolution is 250 solar masses (for the medhighres cases), which is one of the best out there for galaxy simulations containing magnetic fields. While the entire simulation runs over 500 Myr astrophysical timescales, we only upload the final snapshot from both scenarios as they should be equivalent to the present-day LMC. We upload processed quantities, which account for varied radiation background at different places in the interstellar medium, and tools to calculate mock quantities like rotation measures. We also attach one snapshot + processed quantities at low resolution (called medres) for testing.
Contact Email
Hilay.Shah@anu.edu.au
Supervisors
Mark Krumholz; Naomi McClure-Griffiths
Fields of Research
5101 - Astronomical sciences; 510103 - Cosmology and extragalactic astronomy
Socio-Economic Objective
280120 - Expanding knowledge in the physical sciences
Keywords
LMC simulation data; Galaxy simulation; Large Magellanic Cloud; Fluid dynamics; Magnetohydrodynamic simulation
Date of data creation
2025
Year of data publication
2025
Creator(s) for Citation
Shah
Hilay
Krumholz
Mark
McClure-Griffiths
Naomi
Publisher for Citation
The Australian National University Data Commons
Publications
https://doi.org/10.1093/mnras/staf1003
Wind of Change: Faraday Rotation in a Simulated Large Magellanic Cloud
Related Websites
Supercomputing facility
https://nci.org.au/our-systems/hpc-systems
Other Related Identifiers
https://arxiv.org/abs/2503.06449
Access Rights
Open Access allowed. I need ANU Data Commons to host this indefinitely.
Access Rights Type
Open
Retention Period
Indefinitely
Extent or Quantity
6
Data Size
74.2 GB
Status: Published
Published to:
  • Australian National University
  • Australian National Data Service
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