Optical evolution of AT 2024wpp: the high-velocity outflows in Cow-like transients are consistent with high spherical symmetry

• Pursiainen, M.
• Killestein, T.L. https://orcid.org/0000-0002-0440-9597
• Kuncarayakti, H.
• Charalampopoulos, P.
• Warwick, B. https://orcid.org/0009-0005-8379-3871
• Lyman, J. https://orcid.org/0000-0002-3464-0642
• Kotak, R.
• Leloudas, G.
• Coppejans, D.
• Kravtsov, T.
• Maeda, K. https://orcid.org/0000-0003-2611-7269
• Nagao, T. https://orcid.org/0000-0002-3933-7861
• Taguchi, K. https://orcid.org/0000-0002-8482-8993
• Ackley, K.
• Dhillon, V.S. https://orcid.org/0000-0001-5944-4480
• Galloway, D.K.
• Kumar, A. https://orcid.org/0000-0002-4870-9436
• O’Neill, D.
• Ramsay, G. https://orcid.org/0000-0001-8722-9710
• Steeghs, D. https://orcid.org/0000-0003-0771-4746

© 2025 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.

• Published: 7 February 2025
• Published (online): 7 February 2025
• Accepted: 5 February 2025

• Author