Michel, P. D., Mazzali, P. A., Perley, D. A., Hinds, K., & Wise, J. L. (2025). The nebular spectra of SN 2023ixf: A lower mass, partially stripped progenitor may be the result of binary interaction.
Style de citation Chicago (17e éd.)Michel, Philip D., Paolo A. Mazzali, Daniel A. Perley, K-Ryan Hinds, et Jacob L. Wise. The Nebular Spectra of SN 2023ixf: A Lower Mass, Partially Stripped Progenitor May Be the Result of Binary Interaction. 2025.
Style de citation MLA (9e éd.)Michel, Philip D., et al. The Nebular Spectra of SN 2023ixf: A Lower Mass, Partially Stripped Progenitor May Be the Result of Binary Interaction. 2025.
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