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Results of the First Year of the 3BS Polar Search Program
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| dc.contributor.author | Gabdeev M.M. | |
| dc.contributor.author | Fatkhullin T.A. | |
| dc.contributor.author | Borisov N.V. | |
| dc.contributor.author | Shimansky V.V. | |
| dc.contributor.author | Kolbin A.I. | |
| dc.contributor.author | Moskvitin A.S. | |
| dc.contributor.author | Aitov V.N. | |
| dc.contributor.author | Mitiani G.S. | |
| dc.date.accessioned | 2021-02-25T20:37:18Z | |
| dc.date.available | 2021-02-25T20:37:18Z | |
| dc.date.issued | 2020 | |
| dc.identifier.issn | 1063-7737 | |
| dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/162066 | |
| dc.description.abstract | © 2020, Pleiades Publishing, Inc. Abstract: We present the results of the first year of searching for polar candidates within the 3BS (3-Band Survey) program using medium-band filters. Observational data for 84 selected objects from the catalog of cataclysmic variables of the CRTS DR1 sky survey were obtained while implementing the program. A dwarf nova during its outburst and a polar were detected. The available archival data are analyzed. The dwarf nova is of the U Gem or Z Cam type and contains a massive secondary component with M2 = 0.94 ± 0.04 Mʘ. For the polar found we have estimated the orbital period PO = 0d.054437 and calculated the magnetic field strength of the white dwarf B ≈ 32 MG. | |
| dc.relation.ispartofseries | Astronomy Letters | |
| dc.subject | cataclysmic variables | |
| dc.subject | polars | |
| dc.title | Results of the First Year of the 3BS Polar Search Program | |
| dc.type | Article | |
| dc.relation.ispartofseries-issue | 7 | |
| dc.relation.ispartofseries-volume | 46 | |
| dc.collection | Публикации сотрудников КФУ | |
| dc.relation.startpage | 482 | |
| dc.source.id | SCOPUS10637737-2020-46-7-SID85095598488 |
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Публикации сотрудников КФУ Scopus [24551]
Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.