Type Ia supernova explosion models are inherently multidimensional

This is experimental HTML to improve accessibility. We invite you to report rendering errors. Use Alt+Y to toggle on accessible reporting links and Alt+Shift+Y to toggle off. Learn more about this project and help improve conversions.

1 1 institutetext: Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85748, Garching, Germany 2 2 institutetext: School of Science, University of New South Wales, Australian Defence Force Academy, Northcott Drive, Canberra, 2600, ACT, Australia 3 3 institutetext: School of Mathematics and Physics, Queen’s University Belfast, Belfast BT7 1NN, United Kingdom 4 4 institutetext: Heidelberg Institute for Theoretical Studies, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany 5 5 institutetext: Zentrum für Astronomie der Universität Heidelberg, Institut für Theoretische Astrophy

saved by

• Muon Neutrino

related reading

• Predicting the nature of supernova progenitors - PMCpmc.ncbi.nlm.nih.gov
• Type Ia Supernova Light Curves | COSMOSastronomy.swin.edu.au
• The Classification of Supernovae - Astrophysics Data Systemui.adsabs.harvard.edu
• Caltech Scientists Detects First Progenitor of Type 1b Supernova – W. M. Keck Observatorykeckobservatory.org
• Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrumarxiv.org
• [2607.28013] The physical origin of the maximum stellar sizearxiv.org
• [1707.08132] Theoretical Models of Optical Transients. I. A Broad Exploration of the Duration-Luminosity Phase Spacearxiv.org
• Does NGC 6397 contain an intermediate-mass black hole or a more diffuse inner subcluster? | Astronomy & Astrophysics (A&A)aanda.org
• 0903.4186arxiv.org
• The Gaia-ESO survey: New spectroscopic binaries in the Milky Way | Astronomy & Astrophysics (A&A)aanda.org
• Physics of Eclipsing Binaries. VI. Hot, compact starsarxiv.org
• Wolf–Rayet star - Wikipediaen.wikipedia.org