@article{10272/23134,
year = {2018},
url = {https://hdl.handle.net/10272/23134},
abstract = {We report a long-term (1961-2017) study of the eclipse times in the dwarf novae WZ Sagittae, in an effort to learn its rate of orbital-period change. Some wiggles with a timescale of 20-50 years are apparent, and a connection with the ~23 year interval between dwarf-nova eruptions is possible. These back-and-forth wiggles dominate the O-C diagram, and prevent a secure measurement of the steady rate of orbital-period change.},
organization = {National Science Foundation (NSF) grants AST12-11129 y AST16-15456},
publisher = {IOP Publishing},
title = {Orbital period changes in WZ Sagittae},
doi = {10.1088/1538-3873/aaa7e7},
author = {Patterson, Joseph and Stone, Geoffrey and Kemp, Jonathan and Skillman, David and Miguel Agustino, Enrique de and Seargeant, Jim},
}