@article{10272/23132,
year = {2020},
url = {https://hdl.handle.net/10272/23132},
abstract = {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.},
publisher = {Oxford University Press},
title = {Survey of period variations of superhumps in SU UMa-type dwarf novae. X: The tenth year (2017)},
doi = {https://dx.doi.org/10.1093/pasj/psz134},
author = {Kato, Taichi and Isogai, Keisuke and Wakamatsu, Yasuyuki and de Miguel, Enrique and Denisenko, Denis},
}