Photometric and Spectroscopic Study of Two Low Mass Ratio Contact Binary Systems: CRTS J225828.7-121122 and CRTSJ030053.5+230139

The study reports photometric and spectroscopic observations of two recently recognized contact binary systems. Both systems show total eclipses and analysis of the light curves indicates both have very low mass ratios of less than 0.3. We derive absolute parameters from color and distance based cal...

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Veröffentlicht in:Research in astronomy and astrophysics 2023-11, Vol.23 (11), p.115001
Hauptverfasser: Wadhwa, Surjit S., Petrović, Jelena, Tothill, Nick F. H., De Horta, Ain Y., Filipović, Miroslav D., Djurašević, Gojko
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container_issue 11
container_start_page 115001
container_title Research in astronomy and astrophysics
container_volume 23
creator Wadhwa, Surjit S.
Petrović, Jelena
Tothill, Nick F. H.
De Horta, Ain Y.
Filipović, Miroslav D.
Djurašević, Gojko
description The study reports photometric and spectroscopic observations of two recently recognized contact binary systems. Both systems show total eclipses and analysis of the light curves indicates both have very low mass ratios of less than 0.3. We derive absolute parameters from color and distance based calibrations and show that, although both have low mass ratios, they are likely to be in a stable orbit and unlikely to merge. In other respects, both systems have characteristics similar to other contact binaries with the secondary larger and brighter than their main sequence counterparts and we also find that the secondary is considerably denser than the primary in both systems.
doi_str_mv 10.1088/1674-4527/acf445
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subjects (stars:) binaries: eclipsing
Light curve
Mass ratios
Orbital stability
Photometry
Spectroscopic analysis
Spectroscopic observation
stars: mass-loss
techniques: photometric
title Photometric and Spectroscopic Study of Two Low Mass Ratio Contact Binary Systems: CRTS J225828.7-121122 and CRTSJ030053.5+230139
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