SN 2023zaw: The Low-energy Explosion of an Ultrastripped Star

Most stripped-envelope supernova progenitors are thought to be formed through binary interaction, losing hydrogen and/or helium from their outer layers. Ultrastripped supernovae are an emerging class of transient that are expected to be produced through envelope stripping by a neutron star companion...

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Bibliographic Details
Main Authors:	T. Moore, J. H. Gillanders, M. Nicholl, M. E. Huber, S. J. Smartt, S. Srivastav, H. F. Stevance, T.-W. Chen, K. C. Chambers, J. P. Anderson, M. D. Fulton, S. R. Oates, C. Angus, G. Pignata, N. Erasmus, H. Gao, J. Herman, C.-C. Lin, T. Lowe, E. A. Magnier, P. Minguez, C.-C. Ngeow, X. Sheng, S. A. Sim, K. W. Smith, R. Wainscoat, S. Yang, D. R. Young, K.-J. Zeng
Format:	Article
Language:	English
Published:	IOP Publishing 2025-01-01
Series:	The Astrophysical Journal Letters
Subjects:	Transient sources Supernovae Core-collapse supernovae Type Ib supernovae Circumstellar matter
Online Access:	https://doi.org/10.3847/2041-8213/adade6
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SN 2023zaw: The Low-energy Explosion of an Ultrastripped Star

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