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Classical novae and type I X-ray bursts: Challenges for the 21st century

Autor
Parikh, A.R.; Jose, J.; Sala, G.
Tipus d'activitat
Article en revista
Revista
AIP Advances
Data de publicació
2014-04-01
Número
4
DOI
https://doi.org/10.1063/1.4863946 Obrir en finestra nova
Projecte finançador
Physics of compact objects: I.Theorical modeling and observations of stellar explosions
Últimos estadios de la evolución estelar en sistemas binarios: novas clásicas y recurrentes, supernovas, erupciones de rayos X ....
Resum
Classical nova explosions and type I X-ray bursts are the most frequent types of thermonuclear stellar explosions in the Galaxy. Both phenomena arise from thermonuclear ignition in the envelopes of accreting compact objects in close binary star systems. Detailed observations of these events have stimulated numerous studies in theoretical astrophysics and experimental nuclear physics. We discuss observational features of these phenomena and theoretical efforts to better understand the energy prod...
Paraules clau
Novae, Hydrological Modeling, Sodium, Explosions, Element Formation
Grup de recerca
GAA - Grup d'Astronomia i Astrofísica

Participants