PreprintCC BY 4.0arXiv
The light curve modeling of eclipsing cataclysmic variables: from period bouncers to nova-likes
Abstract
I describe the basic concepts used in developing the computer code CVlab V2.0, which simulates the light curves of close binary systems with accretion-disk structures. I provide a detailed description of the code, including its underlying assumptions, limitations, and applications, as well as prospects for future development.
Related
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BibTeX
@misc{zharikov2026light,
title = {{The light curve modeling of eclipsing cataclysmic variables: from period bouncers to nova-likes}},
author = {Sergey Zharikov},
howpublished = {arXiv},
year = {2026},
month = nov,
doi = {10.48550/arxiv.2611.01380},
eprint = {2611.01380},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2611.01380},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - The light curve modeling of eclipsing cataclysmic variables: from period bouncers to nova-likes
AU - Sergey Zharikov
PY - 2026
DA - 2026/11/01
PB - arXiv
DO - 10.48550/arxiv.2611.01380
UR - https://arxiv.org/abs/2611.01380
AB - I describe the basic concepts used in developing the computer code CVlab V2.0, which simulates the light curves of close binary systems with accretion-disk structures. I provide a detailed description of the code, including its underlying assumptions, limitations, and applications, as well as prospects for future development.
ER -