| dc.contributor.author | Orio, M. | |
| dc.contributor.author | Saygac, T. | |
| dc.contributor.author | della Valle, M. | |
| dc.contributor.author | Williams, R. | |
| dc.contributor.author | Bianchini, A. | |
| dc.date.accessioned | 2021-03-03T16:19:30Z | |
| dc.date.available | 2021-03-03T16:19:30Z | |
| dc.identifier.citation | Bianchini A., Saygac T., Orio M., della Valle M., Williams R., "The old nova CP Puppis: a carbon nova and asynchronous polar?", ASTRONOMY & ASTROPHYSICS, cilt.539, 2012 | |
| dc.identifier.issn | 0004-6361 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_43a3c88c-e07b-424e-b52f-a7f65a530b8f | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/49171 | |
| dc.identifier.uri | https://doi.org/10.1051/0004-6361/201117251 | |
| dc.description.abstract | Context. CP Pup (Nova Pup 1942) showed outburst and quiescent characteristics indicating a very massive white dwarf, yet the standard spectroscopic dynamical analysis assuming an accretion disk yields an extremely low value for the white dwarf mass. However, some physical parameters and the accretion geometry are still poorly known. | |
| dc.language.iso | eng | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | Temel Bilimler | |
| dc.subject | Fizik | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Uzay bilimi | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.title | The old nova CP Puppis: a carbon nova and asynchronous polar? | |
| dc.type | Makale | |
| dc.relation.journal | ASTRONOMY & ASTROPHYSICS | |
| dc.contributor.department | University of Padua , , | |
| dc.identifier.volume | 539 | |
| dc.contributor.firstauthorID | 203733 | |
