| dc.contributor.author | DI MILLE, F. | |
| dc.contributor.author | Alis, S. | |
| dc.contributor.author | TAMBURINI, F. | |
| dc.contributor.author | Saygac, Ahmet Talat | |
| dc.contributor.author | Bianchini, A. | |
| dc.date.accessioned | 2021-03-05T15:12:11Z | |
| dc.date.available | 2021-03-05T15:12:11Z | |
| dc.identifier.citation | Bianchini A., DI MILLE F., TAMBURINI F., Saygac A. T. , Alis S., "The Slow Late Decline of the Old Nova RW Ursae Minoris (1956)", 4th International Conference on Classical and Recurrent Novae - Stella Novae: Past and Future Decades, Cape-Town, Güney Afrika, 4 - 08 Şubat 2013, cilt.490, ss.221-224 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_bac96afc-8d56-43b9-8671-762f6708555c | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/124227 | |
| dc.description.abstract | Photometric observations of the old nova RW UMi are presented. Data obtained mostly in the Asiago Observatory of lNAF. The period analysis of the data did not permit to recover the Retter & Lipkin (2001) period. A possible explanation to the nature of QPO in the data is given. | |
| dc.language.iso | eng | |
| dc.subject | Temel Bilimler | |
| dc.subject | Fizik | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Uzay bilimi | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.title | The Slow Late Decline of the Old Nova RW Ursae Minoris (1956) | |
| dc.type | Bildiri | |
| dc.contributor.department | University of Padua , , | |
| dc.identifier.volume | 490 | |
| dc.contributor.firstauthorID | 20801 | |
