CAOSP abstracts, Volume: 55, No.: 3, year: 2025

Author(s): Wolf, M.; Šmecler, L.; Kučáková, H.; Hynek, T.; Zasche, P.; Hornoch, K.; Auer, R.F.
Journal: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 55, no. 3, p. 307-312.
Date: 04/2025
Title: Period changes in low-mass eclipsing binaries: V1828 Aql, NSVS 2676703, and NSVS 6507557
Keyword(s): binaries: eclipsing, binaries: close, stars: low-mass, stars: individual (V1828~Aql, NSVS 2676703, NSVS 6507557)
Pages: 307 -- 312
DOI: https://doi.org/10.31577/caosp.2025.55.3.307
NASA ADS Abstract Service: 2025CoSka..55c.307W
Citation:
License: This work is licensed under a Creative Commons Attribution 4.0 International License

Abstract: Low-mass stars belong to the most numerous component of our Galaxy. We present the new results of our long-term observational project to detect small variations in the orbital periods of low-mass and short-period eclipsing binaries. Three known systems, namely V1828~Aql, NSVS 2676703, NSVS 6507557, and their period changes visible in the current O-C diagrams, are briefly discussed.