Research on the HIP 18856 binary system
The results of a study on the binary HIP 18856 and construction of its orbit are presented. New observational data were obtained at the BTA of SAO RAS in 2007-2019. Earlier, Cvetkovic et al. constructed the orbit for this system. However, it is based on six measurements, which cover a small part of...
Gespeichert in:
| Veröffentlicht in: | Research in astronomy and astrophysics 2021-04, Vol.21 (3), p.58, Article 58 |
|---|---|
| Hauptverfasser: | , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | 3 |
| container_start_page | 58 |
| container_title | Research in astronomy and astrophysics |
| container_volume | 21 |
| creator | Efremova, Polina Mitrofanova, Arina Dyachenko, Vladimir Beskakotov, Anatoly Maksimov, Alexander Rastegaev, Denis Balega, Yury Komarinsky, Sergey |
| description | The results of a study on the binary HIP 18856 and construction of its orbit are presented. New observational data were obtained at the BTA of SAO RAS in 2007-2019. Earlier, Cvetkovic et al. constructed the orbit for this system. However, it is based on six measurements, which cover a small part of the orbit. The positional parameters of the ESA astrometric satellite Hipparcos published speckle interferometric data (Mason et al., Balega et al., Horch et al.) and new ones were used in this study. Based on the new orbital parameters, the mass sum was calculated and the physical parameters of the components were found. The obtained orbital and fundamental parameters were compared with the data from the study by Cvetkovic et al.. The comparison shows that the new orbital solution is better than the old one, since it fits new observational data accurately. Also based on a qualitative evaluation performed by Worley & Heintz, the new orbit was classified as "reliable", which means data cover more than half of the orbit with sufficient quantities of residuals of measurements. |
| doi_str_mv | 10.1088/1674-4527/21/3/058 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2518767942</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2518767942</sourcerecordid><originalsourceid>FETCH-LOGICAL-c275t-2139e0f4a5e278aa647f3393c9be3f958e8efe9da5f5a72e1e34adbebb2d03de3</originalsourceid><addsrcrecordid>eNqNkEtLAzEUhYMoWKt_wNWACxcyTh6T11IGtUJBEV2HzMwNnWInNUmR_nszVLp2de_ifOfecxC6JvieYKUqImRd1pzKipKKVZirEzSjTMtSUKxP0ewoOEcXMa4xFpwLOkO37xDBhm5V-LFIKygWL28FUYqLoh1GG_ZF3McEm0t05uxXhKu_OUefT48fzaJcvj6_NA_LsqOSp5ISpgG72nKgUlkraukY06zTLTCnuQIFDnRvueNWUiDAatu30La0x6wHNkc3B99t8N87iMms_S6M-aShnCgppK5pVtGDqgs-xgDObMOwyd8ags1UiJnymimvocQwkwvJkDpAP9B6F7sBxg6OIJ4qkUxKljdMmiHZNPix8bsxZfTu_yj7BZ2scbo</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2518767942</pqid></control><display><type>article</type><title>Research on the HIP 18856 binary system</title><source>IOP Publishing Journals</source><source>Web of Science - Science Citation Index Expanded - 2021<img src="https://exlibris-pub.s3.amazonaws.com/fromwos-v2.jpg" /></source><source>Alma/SFX Local Collection</source><creator>Efremova, Polina ; Mitrofanova, Arina ; Dyachenko, Vladimir ; Beskakotov, Anatoly ; Maksimov, Alexander ; Rastegaev, Denis ; Balega, Yury ; Komarinsky, Sergey</creator><creatorcontrib>Efremova, Polina ; Mitrofanova, Arina ; Dyachenko, Vladimir ; Beskakotov, Anatoly ; Maksimov, Alexander ; Rastegaev, Denis ; Balega, Yury ; Komarinsky, Sergey</creatorcontrib><description>The results of a study on the binary HIP 18856 and construction of its orbit are presented. New observational data were obtained at the BTA of SAO RAS in 2007-2019. Earlier, Cvetkovic et al. constructed the orbit for this system. However, it is based on six measurements, which cover a small part of the orbit. The positional parameters of the ESA astrometric satellite Hipparcos published speckle interferometric data (Mason et al., Balega et al., Horch et al.) and new ones were used in this study. Based on the new orbital parameters, the mass sum was calculated and the physical parameters of the components were found. The obtained orbital and fundamental parameters were compared with the data from the study by Cvetkovic et al.. The comparison shows that the new orbital solution is better than the old one, since it fits new observational data accurately. Also based on a qualitative evaluation performed by Worley & Heintz, the new orbit was classified as "reliable", which means data cover more than half of the orbit with sufficient quantities of residuals of measurements.</description><identifier>ISSN: 1674-4527</identifier><identifier>EISSN: 2397-6209</identifier><identifier>DOI: 10.1088/1674-4527/21/3/058</identifier><language>eng</language><publisher>BEIJING: Natl Astronomical Observatories, Chin Acad Sciences</publisher><subject>Astronomy & Astrophysics ; Parameters ; Physical properties ; Physical Sciences ; Qualitative analysis ; Satellites ; Science & Technology</subject><ispartof>Research in astronomy and astrophysics, 2021-04, Vol.21 (3), p.58, Article 58</ispartof><rights>Copyright IOP Publishing Apr 2021</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>true</woscitedreferencessubscribed><woscitedreferencescount>1</woscitedreferencescount><woscitedreferencesoriginalsourcerecordid>wos000657377300001</woscitedreferencesoriginalsourcerecordid><citedby>FETCH-LOGICAL-c275t-2139e0f4a5e278aa647f3393c9be3f958e8efe9da5f5a72e1e34adbebb2d03de3</citedby><cites>FETCH-LOGICAL-c275t-2139e0f4a5e278aa647f3393c9be3f958e8efe9da5f5a72e1e34adbebb2d03de3</cites><orcidid>0000-0002-4973-270X</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>315,782,786,27933,27934,39267</link.rule.ids></links><search><creatorcontrib>Efremova, Polina</creatorcontrib><creatorcontrib>Mitrofanova, Arina</creatorcontrib><creatorcontrib>Dyachenko, Vladimir</creatorcontrib><creatorcontrib>Beskakotov, Anatoly</creatorcontrib><creatorcontrib>Maksimov, Alexander</creatorcontrib><creatorcontrib>Rastegaev, Denis</creatorcontrib><creatorcontrib>Balega, Yury</creatorcontrib><creatorcontrib>Komarinsky, Sergey</creatorcontrib><title>Research on the HIP 18856 binary system</title><title>Research in astronomy and astrophysics</title><addtitle>RES ASTRON ASTROPHYS</addtitle><description>The results of a study on the binary HIP 18856 and construction of its orbit are presented. New observational data were obtained at the BTA of SAO RAS in 2007-2019. Earlier, Cvetkovic et al. constructed the orbit for this system. However, it is based on six measurements, which cover a small part of the orbit. The positional parameters of the ESA astrometric satellite Hipparcos published speckle interferometric data (Mason et al., Balega et al., Horch et al.) and new ones were used in this study. Based on the new orbital parameters, the mass sum was calculated and the physical parameters of the components were found. The obtained orbital and fundamental parameters were compared with the data from the study by Cvetkovic et al.. The comparison shows that the new orbital solution is better than the old one, since it fits new observational data accurately. Also based on a qualitative evaluation performed by Worley & Heintz, the new orbit was classified as "reliable", which means data cover more than half of the orbit with sufficient quantities of residuals of measurements.</description><subject>Astronomy & Astrophysics</subject><subject>Parameters</subject><subject>Physical properties</subject><subject>Physical Sciences</subject><subject>Qualitative analysis</subject><subject>Satellites</subject><subject>Science & Technology</subject><issn>1674-4527</issn><issn>2397-6209</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>HGBXW</sourceid><recordid>eNqNkEtLAzEUhYMoWKt_wNWACxcyTh6T11IGtUJBEV2HzMwNnWInNUmR_nszVLp2de_ifOfecxC6JvieYKUqImRd1pzKipKKVZirEzSjTMtSUKxP0ewoOEcXMa4xFpwLOkO37xDBhm5V-LFIKygWL28FUYqLoh1GG_ZF3McEm0t05uxXhKu_OUefT48fzaJcvj6_NA_LsqOSp5ISpgG72nKgUlkraukY06zTLTCnuQIFDnRvueNWUiDAatu30La0x6wHNkc3B99t8N87iMms_S6M-aShnCgppK5pVtGDqgs-xgDObMOwyd8ags1UiJnymimvocQwkwvJkDpAP9B6F7sBxg6OIJ4qkUxKljdMmiHZNPix8bsxZfTu_yj7BZ2scbo</recordid><startdate>20210401</startdate><enddate>20210401</enddate><creator>Efremova, Polina</creator><creator>Mitrofanova, Arina</creator><creator>Dyachenko, Vladimir</creator><creator>Beskakotov, Anatoly</creator><creator>Maksimov, Alexander</creator><creator>Rastegaev, Denis</creator><creator>Balega, Yury</creator><creator>Komarinsky, Sergey</creator><general>Natl Astronomical Observatories, Chin Acad Sciences</general><general>IOP Publishing</general><scope>BLEPL</scope><scope>DTL</scope><scope>HGBXW</scope><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/0000-0002-4973-270X</orcidid></search><sort><creationdate>20210401</creationdate><title>Research on the HIP 18856 binary system</title><author>Efremova, Polina ; Mitrofanova, Arina ; Dyachenko, Vladimir ; Beskakotov, Anatoly ; Maksimov, Alexander ; Rastegaev, Denis ; Balega, Yury ; Komarinsky, Sergey</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c275t-2139e0f4a5e278aa647f3393c9be3f958e8efe9da5f5a72e1e34adbebb2d03de3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Astronomy & Astrophysics</topic><topic>Parameters</topic><topic>Physical properties</topic><topic>Physical Sciences</topic><topic>Qualitative analysis</topic><topic>Satellites</topic><topic>Science & Technology</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Efremova, Polina</creatorcontrib><creatorcontrib>Mitrofanova, Arina</creatorcontrib><creatorcontrib>Dyachenko, Vladimir</creatorcontrib><creatorcontrib>Beskakotov, Anatoly</creatorcontrib><creatorcontrib>Maksimov, Alexander</creatorcontrib><creatorcontrib>Rastegaev, Denis</creatorcontrib><creatorcontrib>Balega, Yury</creatorcontrib><creatorcontrib>Komarinsky, Sergey</creatorcontrib><collection>Web of Science Core Collection</collection><collection>Science Citation Index Expanded</collection><collection>Web of Science - Science Citation Index Expanded - 2021</collection><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>Efremova, Polina</au><au>Mitrofanova, Arina</au><au>Dyachenko, Vladimir</au><au>Beskakotov, Anatoly</au><au>Maksimov, Alexander</au><au>Rastegaev, Denis</au><au>Balega, Yury</au><au>Komarinsky, Sergey</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Research on the HIP 18856 binary system</atitle><jtitle>Research in astronomy and astrophysics</jtitle><stitle>RES ASTRON ASTROPHYS</stitle><date>2021-04-01</date><risdate>2021</risdate><volume>21</volume><issue>3</issue><spage>58</spage><pages>58-</pages><artnum>58</artnum><issn>1674-4527</issn><eissn>2397-6209</eissn><abstract>The results of a study on the binary HIP 18856 and construction of its orbit are presented. New observational data were obtained at the BTA of SAO RAS in 2007-2019. Earlier, Cvetkovic et al. constructed the orbit for this system. However, it is based on six measurements, which cover a small part of the orbit. The positional parameters of the ESA astrometric satellite Hipparcos published speckle interferometric data (Mason et al., Balega et al., Horch et al.) and new ones were used in this study. Based on the new orbital parameters, the mass sum was calculated and the physical parameters of the components were found. The obtained orbital and fundamental parameters were compared with the data from the study by Cvetkovic et al.. The comparison shows that the new orbital solution is better than the old one, since it fits new observational data accurately. Also based on a qualitative evaluation performed by Worley & Heintz, the new orbit was classified as "reliable", which means data cover more than half of the orbit with sufficient quantities of residuals of measurements.</abstract><cop>BEIJING</cop><pub>Natl Astronomical Observatories, Chin Acad Sciences</pub><doi>10.1088/1674-4527/21/3/058</doi><tpages>4</tpages><orcidid>https://orcid.org/0000-0002-4973-270X</orcidid></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1674-4527 |
| ispartof | Research in astronomy and astrophysics, 2021-04, Vol.21 (3), p.58, Article 58 |
| issn | 1674-4527 2397-6209 |
| language | eng |
| recordid | cdi_proquest_journals_2518767942 |
| source | IOP Publishing Journals; Web of Science - Science Citation Index Expanded - 2021<img src="https://exlibris-pub.s3.amazonaws.com/fromwos-v2.jpg" />; Alma/SFX Local Collection |
| subjects | Astronomy & Astrophysics Parameters Physical properties Physical Sciences Qualitative analysis Satellites Science & Technology |
| title | Research on the HIP 18856 binary system |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-02T12%3A54%3A50IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Research%20on%20the%20HIP%2018856%20binary%20system&rft.jtitle=Research%20in%20astronomy%20and%20astrophysics&rft.au=Efremova,%20Polina&rft.date=2021-04-01&rft.volume=21&rft.issue=3&rft.spage=58&rft.pages=58-&rft.artnum=58&rft.issn=1674-4527&rft.eissn=2397-6209&rft_id=info:doi/10.1088/1674-4527/21/3/058&rft_dat=%3Cproquest_cross%3E2518767942%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2518767942&rft_id=info:pmid/&rfr_iscdi=true |