Please use this identifier to cite or link to this item:
https://research.matf.bg.ac.rs/handle/123456789/3002| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Novaković, Bojan | en_US |
| dc.date.accessioned | 2025-12-12T18:19:32Z | - |
| dc.date.available | 2025-12-12T18:19:32Z | - |
| dc.date.issued | 2008-02 | - |
| dc.identifier.uri | https://research.matf.bg.ac.rs/handle/123456789/3002 | - |
| dc.description.abstract | We present here the orbital elements for the pair BC of visual binary star WDS 18253+4846 (ADS 11344 = HD 170109) and ephemerides for the period 2008-2014. As the orbital elements of pair AB already existed we analyzed mass ratio between these two pairs and concluded that components C is the biggest one in this triple system. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Observatory, Rutherford Appleton Lab, Oxford | en_US |
| dc.relation.ispartof | The Observatory | en_US |
| dc.title | A possible orbital solution for the triple star WDS 18253+4846 | en_US |
| dc.type | Contribution to Journal | en_US |
| dc.identifier.doi | 10.48550/arXiv.0710.3601 | - |
| dc.identifier.isi | 000253662000005 | - |
| dc.identifier.url | http://dx.doi.org/10.48550/arXiv.0710.3601 | - |
| dc.contributor.affiliation | Astronomy | en_US |
| dc.relation.issn | 0029-7704 | en_US |
| dc.description.rank | M23 | en_US |
| dc.relation.firstpage | 56 | en_US |
| dc.relation.lastpage | 57 | en_US |
| dc.relation.volume | 128 | en_US |
| dc.relation.issue | 1202 | en_US |
| item.openairetype | Contribution to Journal | - |
| item.languageiso639-1 | en | - |
| item.grantfulltext | none | - |
| item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
| item.fulltext | No Fulltext | - |
| item.cerifentitytype | Publications | - |
| crisitem.author.dept | Astronomy | - |
| crisitem.author.orcid | 0000-0001-6349-6881 | - |
| Appears in Collections: | Research outputs | |
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