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View article: Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagittarii
Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagittarii Open
Context. The overwhelming majority of cataclysmic variables (CVs) have orbital periods shorter than 10 h. However, a few have much longer orbital periods, and their formation and existence pose certain challenges for the CV evolution model…
View article: Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagitarii
Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagitarii Open
The overwhelming majority of CVs have orbital periods shorter than 10 hr. However, a few have much longer periods, and their formation and existence pose challenges for the CV evolution models. These extremely long-period CVs must host nuc…