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 |
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container_issue | 11 |
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container_title | Research in astronomy and astrophysics |
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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 |
format | Article |
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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.</description><subject>(stars:) binaries: eclipsing</subject><subject>Light curve</subject><subject>Mass ratios</subject><subject>Orbital stability</subject><subject>Photometry</subject><subject>Spectroscopic analysis</subject><subject>Spectroscopic observation</subject><subject>stars: mass-loss</subject><subject>techniques: photometric</subject><issn>1674-4527</issn><issn>2397-6209</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><recordid>eNp1kMtLAzEQxoMoWB93jwEvgm6bTB678abFJxXF1nNI0wS32GbdpJTe_NNNrehFh4GBmW--YX4IHVHSpaSqelSWvOACyp6xnnOxhTrAVFlIIGobdX7Gu2gvxikhUggJHfTx9BpSmLnU1hab-QQPG2dTG6INTe4M02KywsHj0TLgQVjiBxMjfjapDrgf5snYhC_ruWlXeLiKyc3iOe4_j4b4HkBUUHXLggKlAF_e68k9YYQI1hWnwAhl6gDtePMW3eF33Ucv11ej_m0xeLy5618MCguKp6IypVGOeyKlcib_oSyVzlnOxt4DGYPKwQCgFEyWTljuKbNgBDPej92Y7aPjjW_ThveFi0lPw6Kd55MaqhKUIJJXWUU2KpsRxNZ53bT1LL-nKdFrznoNUq9B6g3nvHKyWalD8-vZGqOBaUpzCkKobiY-S8_-kP7r_AkBwYa8</recordid><startdate>20231101</startdate><enddate>20231101</enddate><creator>Wadhwa, Surjit S.</creator><creator>Petrović, Jelena</creator><creator>Tothill, Nick F. H.</creator><creator>De Horta, Ain Y.</creator><creator>Filipović, Miroslav D.</creator><creator>Djurašević, Gojko</creator><general>National Astromonical Observatories, CAS and IOP Publishing</general><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-7011-7541</orcidid></search><sort><creationdate>20231101</creationdate><title>Photometric and Spectroscopic Study of Two Low Mass Ratio Contact Binary Systems: CRTS J225828.7-121122 and CRTSJ030053.5+230139</title><author>Wadhwa, Surjit S. ; Petrović, Jelena ; Tothill, Nick F. 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H.</creatorcontrib><creatorcontrib>De Horta, Ain Y.</creatorcontrib><creatorcontrib>Filipović, Miroslav D.</creatorcontrib><creatorcontrib>Djurašević, Gojko</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Research in astronomy and astrophysics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wadhwa, Surjit S.</au><au>Petrović, Jelena</au><au>Tothill, Nick F. H.</au><au>De Horta, Ain Y.</au><au>Filipović, Miroslav D.</au><au>Djurašević, Gojko</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Photometric and Spectroscopic Study of Two Low Mass Ratio Contact Binary Systems: CRTS J225828.7-121122 and CRTSJ030053.5+230139</atitle><jtitle>Research in astronomy and astrophysics</jtitle><stitle>RAA</stitle><addtitle>Res. Astron. Astrophys</addtitle><date>2023-11-01</date><risdate>2023</risdate><volume>23</volume><issue>11</issue><spage>115001</spage><pages>115001-</pages><issn>1674-4527</issn><eissn>2397-6209</eissn><coden>RAAEBW</coden><abstract>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.</abstract><cop>Beijing</cop><pub>National Astromonical Observatories, CAS and IOP Publishing</pub><doi>10.1088/1674-4527/acf445</doi><tpages>6</tpages><orcidid>https://orcid.org/0000-0002-7011-7541</orcidid></addata></record> |
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source | Institute of Physics Journals; Alma/SFX Local Collection |
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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