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Recent advances in the modelling of classical novae and type I X-ray bursts

Autor
Jose, J.; Casanova, J.; Parikh, A.R.; Garcia-berro, E.
Tipus d'activitat
Article en revista
Revista
Journal of physics: conference series
Data de publicació
2012
Volum
337
Pàgina inicial
012038 -1
Pàgina final
012038 - 6
DOI
https://doi.org/10.1088/1742-6596/337/1/012038 Obrir en finestra nova
Repositori
http://hdl.handle.net/2117/16412 Obrir en finestra nova
URL
http://iopscience.iop.org/1742-6596/337/1/012038/pdf/1742-6596_337_1_012038.pdf Obrir en finestra nova
Resum
Classical nova outbursts and type I X-ray bursts are thermonuclear stellar explosions driven by charged-particle reactions. Extensive numerical simulations of nova explosions have shown that the accreted envelopes attain peak temperatures between 0.1 and 0.4 GK, for about several hundred seconds, and therefore, their ejecta is expected to show signatures of significant nuclear activity. Indeed, it has been claimed that novae play some role in the enrichment of the interstellar medium through a n...
Citació
José, J. [et al.]. Recent advances in the modelling of classical novae and type I X-ray bursts. "Journal of Physics: Conference Series", 2012, vol. 337, p. 1-7.
Paraules clau
Accreting neutron-stars, Grains, Nucleosynthesis, Outbursts, RP-process
Grup de recerca
GAA - Grup d'Astronomia i Astrofísica

Participants

  • José Pont, Jordi  (autor)
  • Casanova Bustamante, Jordi  (autor)
  • Parikh, Anuj Ramesh  (autor)
  • Garcia-berro Montilla, Enrique  (autor)

Arxius