Multiple outflows and delayed ejections revealed by early imaging of novae
Elias Aydi, John D. Monnier, Antoine M’erand, Gail H. Schaefer, Laura Chomiuk, Magdalena Otulakowska-Hypka, Jhih-Ling Fan, Kwan Lok Li, Kirill V. Sokolovsky, Ricardo Salinas, Michael Tucker, Benjamin Shappee, Richard Rudy, Kim L. Page, N. Paul M. Kuin, David A. H. Buckley, Peter Craig, Luca Izzo, Justin Linford, Brian D. Metzger, Koji Mukai, Marina Orio, Ken J. Shen, Jay Strader, Jennifer L. Sokoloski, Robert E. Williams, Montana N. Williams, Gesesew R. Habtie, Stefan Kraus, Narsireddy Anugu, Jean-Baptiste Le Bouquin, Sorabh Chhabra, Isabelle Codron, Tyler Gardner, Mayra Gutierrez, Noura Ibrahim, Cyprien Lanthermann, Benjamin R. Setterholm, Christopher Ashall, Jason T. Hinkle, Thomas de Jaeger, Anna V. Payne
arXiv:2512.05220v1 Announce Type: new
Abstract: Novae are thermonuclear eruptions on accreting white dwarfs in interacting binaries. Although most of the accreted envelope is expelled, the mechanism — impulsive ejection, multiple outflows or prolonged winds, or a common-envelope interaction — remains uncertain. GeV $gamma$-ray detections from $>20$ Galactic novae establish these eruptions as nearby laboratories for shock physics and particle acceleration, underscoring the need to determine how novae eject their envelopes. Here we report on near-infrared interferometry, supported with multiwavelength observations, of two $gamma$-ray detected novae. The images of the very fast 2021 nova V1674~Her, taken just 2–3 days after discovery, reveal the presence of two perpendicular outflows. The interaction between these outflows likely drives the observed $gamma$-ray emission. Conversely, the images of the very slow 2021 nova V1405~Cas suggest a delay in the ejection of the bulk of the accreted envelope of more than 50 days after the start of eruption, as the nova slowly rises to visible peak and during which the envelope engulfed the system in a common envelope phase. These unprecedented images offer direct observational evidence that the mechanisms driving mass ejection from the surfaces of accreting white dwarfs are not as simple as previously thought, revealing multiple outflows and delayed ejections.arXiv:2512.05220v1 Announce Type: new
Abstract: Novae are thermonuclear eruptions on accreting white dwarfs in interacting binaries. Although most of the accreted envelope is expelled, the mechanism — impulsive ejection, multiple outflows or prolonged winds, or a common-envelope interaction — remains uncertain. GeV $gamma$-ray detections from $>20$ Galactic novae establish these eruptions as nearby laboratories for shock physics and particle acceleration, underscoring the need to determine how novae eject their envelopes. Here we report on near-infrared interferometry, supported with multiwavelength observations, of two $gamma$-ray detected novae. The images of the very fast 2021 nova V1674~Her, taken just 2–3 days after discovery, reveal the presence of two perpendicular outflows. The interaction between these outflows likely drives the observed $gamma$-ray emission. Conversely, the images of the very slow 2021 nova V1405~Cas suggest a delay in the ejection of the bulk of the accreted envelope of more than 50 days after the start of eruption, as the nova slowly rises to visible peak and during which the envelope engulfed the system in a common envelope phase. These unprecedented images offer direct observational evidence that the mechanisms driving mass ejection from the surfaces of accreting white dwarfs are not as simple as previously thought, revealing multiple outflows and delayed ejections.