Published October 11, 2019
| Version 1.0
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Animations for "Remnants of Subdwarf Helium Donor Stars Ejected from Close Binaries with Thermonuclear Supernovae"
Authors/Creators
- 1. Kavli Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106, USA
- 2. Department of Physics, University of California, Santa Barbara, CA 93106, USA
Description
Movies showing time evolution of the density in the z=0 plane for each of the seven Athena++ models in the paper. Each movie file corresponds to one model, labeled according to donor model number and the kinetic energy of the explosion in units of 1051 ergs.
Notes
Upload performed by an AAS Journals Data Editor
Files
ReadMe.txt
Files
(15.8 MB)
| Name | Size | Download all |
|---|---|---|
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md5:db12378b28cf2de6fcff95a4a717bcf1
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1.9 MB | Download |
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md5:6bd25992eb8303cea7ae6bd40dcd5419
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1.9 MB | Download |
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md5:89656c5f1862fef2db4a1417ed287ca2
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2.1 MB | Download |
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md5:8a7d8c2b1feb4add2ad74622d06e9bd2
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3.0 MB | Download |
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md5:ec489fcf7dee3fcad5903793bb927594
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2.9 MB | Download |
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md5:7d01067955a31013ce53ee18f3c1f98e
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2.4 MB | Download |
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md5:be4468f97f1b733e86c65545e3f2edeb
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1.6 MB | Download |
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md5:328f4a1d54cb5f9e5fce629aab398664
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1.4 kB | Preview Download |
Additional details
Related works
- Is supplement to
- Preprint: arXiv:1906.08941 (arXiv)
- Journal article: 10.3847/1538-4357/ab4ea4 (DOI)