Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Camps magnètics solars"'
Autor:
Niranjan C. Roy, Vishal Tiwari, Alexey Bobrick, Daniel Kosakowski, Robert Fisher, Hagai B. Perets, Rahul Kashyap, Pablo Lorén-Aguilar, Enrique García-Berro
Publikováno v:
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Universitat Politècnica de Catalunya (UPC)
The origins of type Ia supernovae (SNe Ia) are still debated. Some of the leading scenarios involve a double detonation in double white dwarf (WD) systems. In these scenarios, helium shell detonation occurs on top of a carbon-oxygen (CO) WD, which th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88b8b8e4d2ca156466ce401585af44e9
http://arxiv.org/abs/2204.09683
http://arxiv.org/abs/2204.09683
Publikováno v:
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Recercat. Dipósit de la Recerca de Catalunya
instname
Universitat Politècnica de Catalunya (UPC)
Recercat. Dipósit de la Recerca de Catalunya
instname
Isolated magnetic white dwarfs have field strengths ranging from kilogauss to gigagauss. However, the origin of the magnetic field has not been hitherto elucidated. Whether these fields are fossil, hence the remnants of original weak magnetic fields
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c23b510a178d78b3ebf66aa9750e2c8
Publikováno v:
Recercat. Dipósit de la Recerca de Catalunya
instname
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
instname
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Isolated magnetic white dwarfs have field strengths ranging from kilogauss to gigagauss, and constitute an interesting class of objects. The origin of the magnetic field is still the subject of a hot debate. Whether these fields are fossil, hence the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ca2fa809267ff4079a56e34bdcf380d
https://doi.org/10.1142/s0218271816300056
https://doi.org/10.1142/s0218271816300056
