Period changes in low-mass eclipsing binaries: V1828 Aql, NSVS
2676703, and NSVS 6507557

J 2025

Period changes in low-mass eclipsing binaries: V1828 Aql, NSVS 2676703, and NSVS 6507557

WOLF, M.; L. SMECLER; Hana KUČÁKOVÁ; T. HYNEK; P. ZASCHE et al.

Basic information

Original name

Period changes in low-mass eclipsing binaries: V1828 Aql, NSVS 2676703, and NSVS 6507557

Authors

WOLF, M.; L. SMECLER; Hana KUČÁKOVÁ; T. HYNEK; P. ZASCHE; K. HORNOCH and R. F. AUER

Edition

CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO, 2025, 1335-1842

Other information

Language

English

Type of outcome

Article in a journal

Field of Study

10308 Astronomy

Country of publisher

Slovakia

Confidentiality degree

is not subject to a state or trade secret

References:

URL

Impact factor

Impact factor: 0.200 in 2024

Organization unit

Institute of physics in Opava

DOI

https://doi.org/10.31577/caosp.2025.55.3.307

UT WoS

001509136400029

EID Scopus

2-s2.0-105005969511

Keywords in English

binaries;eclipsing-binaries;close-star;slow-mass;stars: individual (V1828 Aql; NSVS 2676703; NSVS 6507557)

Abstract

In the original language

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.

Cite

WOLF, M.; L. SMECLER; Hana KUČÁKOVÁ; T. HYNEK; P. ZASCHE; K. HORNOCH and R. F. AUER. Period changes in low-mass eclipsing binaries: V1828 Aql, NSVS 2676703, and NSVS 6507557. CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO. 2025, vol. 55, No 3, p. 307-312. ISSN 1335-1842. Available from: https://doi.org/10.31577/caosp.2025.55.3.307.

@article{90376,
   author = {Wolf, M. and Smecler, L. and Kučáková, Hana and Hynek, T. and Zasche, P. and Hornoch, K. and Auer, R. F.},
   article_number = {3},
   doi = {https://doi.org/10.31577/caosp.2025.55.3.307},
   keywords = {binaries;eclipsing-binaries;close-star;slow-mass;stars: individual (V1828 Aql; NSVS 2676703; NSVS 6507557)},
   language = {eng},
   issn = {1335-1842},
   journal = {CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO},
   title = {Period changes in low-mass eclipsing binaries: V1828 Aql, NSVS 2676703, and NSVS 6507557},
   url = {https://www.astro.sk/caosp/Eedition/FullTexts/vol55no3/pp307-312.pdf?utm_source=clarivate&getft_integrator=clarivate},
   volume = {55},
   year = {2025}
}

TY  - JOUR
ID  - 90376
AU  - Wolf, M. - Smecler, L. - Kučáková, Hana - Hynek, T. - Zasche, P. - Hornoch, K. - Auer, R. F.
PY  - 2025
TI  - Period changes in low-mass eclipsing binaries: V1828 Aql, NSVS 2676703, and NSVS 6507557
JF  - CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO
VL  - 55
IS  - 3
SP  - 307-312
EP  - 307-312
SN  - 13351842
KW  - binaries;eclipsing-binaries;close-star;slow-mass;stars: individual (V1828 Aql
KW  - NSVS 2676703
KW  - NSVS 6507557)
UR  - https://www.astro.sk/caosp/Eedition/FullTexts/vol55no3/pp307-312.pdf?utm_source=clarivate&getft_integrator=clarivate
N2  - 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.
ER  -

WOLF, M.; L. SMECLER; Hana KUČÁKOVÁ; T. HYNEK; P. ZASCHE; K. HORNOCH and R. F. AUER. Period changes in low-mass eclipsing binaries: V1828 Aql, NSVS 2676703, and NSVS 6507557. \textit{CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO}. 2025, vol.~55, No~3, p.~307-312. ISSN~1335-1842. Available from: https://doi.org/10.31577/caosp.2025.55.3.307.

Přehled o publikaci