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)

Tags

RIV26, UF

Tags

International impact, Reviewed
Changed: 26/1/2026 13:04, Mgr. Pavlína Jalůvková

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.
Displayed: 30/1/2026 08:20