Kato, TaichiIsogai, KeisukeWakamatsu, Yasuyukide Miguel, EnriqueDenisenko, Denis2024-02-062024-02-062020Kato, T., Isogai, K., Wakamatsu, Y., Hambsch, F.-J., Itoh, H., Tordai, T., Vanmunster, T., Dubovsky, P. A., Kudzej, I., Medulka, T., Kimura, M., Ohnishi, R., Monard, B., Pavlenko, E. P., Antonyuk, K. A., Pit, N. V., Antonyuk, O. I., Babina, J. V., Baklanov, A. V., … Denisenko, D. (2020). Survey of period variations of superhumps in SU UMa-type dwarf novae. X. The tenth year (2017). In Publications of the Astronomical Society of Japan (Vol. 72, Issue 1). Oxford University Press (OUP). https://doi.org/10.1093/pasj/psz1340004-62642053-051X (electrónico)https://hdl.handle.net/10272/23132Por recomendación de la oficina editorial, toda la parte de resultados se publicó en la sección Supporting Information (SI) de la revista PASJ (Supplementary data).Continuing the project described by Kato et al. (2009, PASJ, 61, S395), we collected times of superhump maxima for 102 SU UMa-type dwarf novae observed mainly during the 2017 season, and characterized these objects. WZ Sge-type stars identified in this study are PT And, ASASSN-17ei, ASASSN-17el, ASASSN-17es, ASASSN-17fn, ASASSN-17fz, ASASSN-17hw, ASASSN-17kd, ASASSN-17la, PNV J20205397+2508145, and TCP J00332502-3518565. We obtained new mass ratios for seven objects using growing superhumps (stage A). ASASSN-17gf is an EI Psc-type object below the period minimum. CRTS J080941.3+171528 and DDE 51 are objects in the period gap, and both showed a long-lasting phase of stage A superhumps. We also summarize the recent advances in understanding of SU UMa-type and WZ Sge-type dwarf novae.engAtribución-NoComercial-SinDerivadas 3.0 Españahttp://creativecommons.org/licenses/by-nc-nd/3.0/es/accretion, accretion disksstars: dwarf novaestars: novae, cataclysmic variablesjournal articlehttps://dx.doi.org/10.1093/pasj/psz134open access21 Astronomía y Astrofísica