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Table · dataset · 2025

V1141 Cas UBVRI(RI)c light curves

Listed in IVOA Registry (Virtual Observatory)

High-precision photometric measurements of the unexplored eclipsing star V1141 Cas (P=6.909d, V=12.02mag, e=0.37, Sp=B1 V) have shown that the apsidal rotation velocity, dw/dt=0.127 deg/yr is two times slower than the theoretical value under the synchronism condition, dw/dt=0.235deg/yr.

Description

The physical parameters of the component stars were obtained: T1=23500+/-400K, M1=(8.4+/-0.5)M_{sun}_, R1=(4.24+/-0.08)R_{sun}_, T2=22000+/-400K, M2=(7.0+/-0.5)M_{sun}_, R2=(3.38+/-0.08)R_{sun}_.

The age of the system is determined to be 7.5 mln years for a solar chemical composition. The measured photometric parallax, pi=0.00031"+/-0.00004", is very close to the Gaia value. The interstellar extinction, Av=2.2mag, is 40 percent higher than the survey's data.

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Topics

Stated by source
Infrared · Optical
Provenance · 1 source records, 9 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/other/arep/69.69415 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:infraredsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:opticalsource · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0