Astronomers have successfully imaged a nova in unprecedented detail, revealing that the event was not a single explosion, but rather a complex interplay of multiple ejecta flows. The images were captured using the Center for High Angular Resolution Astronomy (CHARA Array) at Georgia State University's near-infrared interferometry technique.
The observations focused on two novae: V1674 Herculis and V1405 Cassiopeiae. V1674 was one of the fastest novas ever recorded, peaking in brightness just 16 hours after its discovery and fading rapidly within a few days. In contrast, V1405 took 53 days to reach its peak brightness and remained bright for approximately 200 days.
The high-resolution images of V1674 show an explosion with two distinct ejecta flows - one moving northwest and the other southeast, with an elliptical structure radiating almost perpendicular to them. This suggests that multiple ejecta streams interacted during the event.
Furthermore, spectroscopic observations revealed different velocity components in the hydrogen atoms' Balmer series, indicating a complex interaction between the various ejecta streams. These findings are significant as they provide direct evidence of high-energy gamma rays and powerful shock waves formed by the collision of these streams.
V1405's observations were equally remarkable, with initial images showing only a bright central light source and few surrounding ejections. However, subsequent observations revealed dramatic changes in the structure, with new ejecta flows emerging and generating shock waves that released material into space.
The study demonstrates that novae are far more complex than initially thought, serving as "laboratories" for studying shock waves and particle acceleration. The team's findings offer a deeper understanding of these astronomical phenomena and their potential to provide insights into the universe's most dramatic events.
The observations focused on two novae: V1674 Herculis and V1405 Cassiopeiae. V1674 was one of the fastest novas ever recorded, peaking in brightness just 16 hours after its discovery and fading rapidly within a few days. In contrast, V1405 took 53 days to reach its peak brightness and remained bright for approximately 200 days.
The high-resolution images of V1674 show an explosion with two distinct ejecta flows - one moving northwest and the other southeast, with an elliptical structure radiating almost perpendicular to them. This suggests that multiple ejecta streams interacted during the event.
Furthermore, spectroscopic observations revealed different velocity components in the hydrogen atoms' Balmer series, indicating a complex interaction between the various ejecta streams. These findings are significant as they provide direct evidence of high-energy gamma rays and powerful shock waves formed by the collision of these streams.
V1405's observations were equally remarkable, with initial images showing only a bright central light source and few surrounding ejections. However, subsequent observations revealed dramatic changes in the structure, with new ejecta flows emerging and generating shock waves that released material into space.
The study demonstrates that novae are far more complex than initially thought, serving as "laboratories" for studying shock waves and particle acceleration. The team's findings offer a deeper understanding of these astronomical phenomena and their potential to provide insights into the universe's most dramatic events.