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 \(M_{2}=0.94\pm 0.04M_{\odot}\). For the polar found we have estimated the orbital period \(P_{O}=0\overset{d}{.}054437\) and calculated the magnetic field strength of the white dwarf \(B\approx 32\) MG.
Similar content being viewed by others
Notes
https://www.sao.ru/3BS/.
http://nesssi.cacr.caltech.edu/catalina/20131014/ 1310141400044134796.html.
http://dr4.lamost.org/spectrum/view?obsid=279513203.
http://nunuku.caltech.edu/cgi-bin/getcssconedb_release_ img.cgi.
http://nesssi.cacr.caltech.edu/catalina/20110920/ 1109201210794130197.html.
http://skyserver.sdss.org/dr12/en/get/SpecById.ashx?id= 4446402577529761792.
http://www.vgoranskij.net/software/.
REFERENCES
J. A. Bailey, L. Ferrario, D. T. Wickramasinghe, et al., Mon. Not. R. Astron. Soc. 272, 579 (1995).
E. Bertin, Astron. Data Anal. Software Syst. XX 442, 435 (2011).
E. Bertin and S. Arnouts, Astron. Astrophys. Suppl. Ser. 117, 393 (1996).
K. Buermann and H.-C. Thomas, Adv. Space Res. 13, 115 (1993).
M. Cropper, Space Sci. Rev. 54, 195 (1990).
A. J. Drake, S. G. Djorgovski, A. Mahabal, et al., Astrophys. J. 696, 870 (2009).
A. J. Drake, B. T. Gänsicke, S. G. Djorgovski, et al., Mon. Not. R. Astron. Soc. 441, 1186 (2014).
E. V. Emelyanov, T. A. Fatkhullin, and A. S. Moskvitin, SAO RAN Tech. Report No. 340 (Spets. Astrophys. Observ. RAS, Zelenchuk, 2019).
M. M. Gabdeev, T. A. Fatkhullin, and N. V. Borisov, arXiv:2004.11764 (2020).
L. Girardi, A. Bressan, G. Bertelli, et al., Astron. Astrophys. Suppl. Ser. 141, 371 (2000).
M. Honda, K. Osawa, K. Osada, et al., IAU Circ. 2826, 1 (1975).
W. Hou, A.-Li Luo, Yin Bi Li, et al., Astron. J. 159, 18 (2020).
A. I. Kolbin, N. A. Serebryakova, M. M. Gabdeev, et al., Astrophys. Bull. 74, 80 (2019).
J. Lafler and T. D. Kinman, Astrophys. J. Suppl. Ser. 11, 216 (1965).
D. Lang, D. W. Hogg, K. Mierle, et al., Astron. J. 139, 1782 (2010).
L. Morales-Rueda and T. R. Marsh, Mon. Not. R. Astron. Soc. 332, 814 (2002).
P. Mróz, A. Udalski, R. Poleski, et al., Acta Astron. 65, 313 (2015).
H. Ritter and U. Kolb, Astron. Astrophys. 404, 301 (2004).
S. R. Rosen, N. A. Webb, M. G. Watson, et al., Astron. Astrophys. 590, A1 (2016).
H. S. Stockman, G. D. Schmidt, and D. Q. Lamb, Astrophys. J. 332, 282 (1988).
P. Szkody, S. F. Anderson, K. Brooks, et al., Astron. J. 142, 181 (2011).
B. Warner, in Cataclysmic Variable Stars (Cambridge Univ. Press, Cambridge, 2003), p. 307.
G. Williams and W. A. Hiltner, Astrophys. J. 252, 277 (1982).
S. Zhang, A.-L. Luo, G. Comte, et al., VizieR Online Data Catalog J/ApJS/240/31 (2019).
Funding
This work is based on the observational data obtained at the Zeiss-1000 SAO RAS telescope under the support of the Ministry of Science and Higher Education of the Russian Federation (including contract no. 05.619.21.0016, unique project identifierRFMEFI61919X0016). The study was financially supported by the Russian Science Foundation (RSF no. 18-72-00106). V.N. Aitov thanks the Russian Foundation for Basic Research (project no. 18-29-21030) for the support of his participation in the observations. V.V. Shimansky thanks the Russian Foundation for Basic Research (project no. 18-42-160003).
Author information
Authors and Affiliations
Corresponding author
Additional information
Translated by V. Astakhov
Rights and permissions
About this article
Cite this article
Gabdeev, M.M., Fatkhullin, T.A., Borisov, N.V. et al. Results of the First Year of the 3BS Polar Search Program. Astron. Lett. 46, 482–487 (2020). https://doi.org/10.1134/S1063773720060031
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1063773720060031