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

TL;DR
This study uses early imaging and multiwavelength observations of two gamma-ray detected novae to reveal complex ejection mechanisms, including multiple outflows and delayed envelope ejections, challenging previous simplified models.
Contribution
It provides the first direct observational evidence of multiple outflows and delayed ejections in novae, highlighting complex mass ejection processes.
Findings
Fast nova V1674 Her shows two perpendicular outflows.
Slow nova V1405 Cas exhibits delayed ejection over 50 days.
Interaction of outflows likely causes gamma-ray emission.
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 -ray detections from 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 -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 -ray emission. Conversely, the images of the very slow 2021 nova V1405~Cas…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
