A Possible Orbital Solution For The Triple Star WDS 18253+4846
| dc.creator | Novakovic, Bojan | |
| dc.date | 2007-10-18 | |
| dc.date | 2008-02-04 | |
| dc.date.accessioned | 2026-07-07T09:18:08Z | |
| dc.date.available | 2026-07-07T09:18:08Z | |
| dc.description | 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. | |
| dc.description | Accepted for publication in "The Observatory" v3 - references added | |
| dc.identifier | https://arxiv.org/abs/0710.3601 | |
| dc.identifier | http://arxiv.org/abs/0710.3601 | |
| dc.identifier | The Observatory, Vol. 128, p. 56, 2008 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/153918 | |
| dc.subject | Astrophysics | |
| dc.title | A Possible Orbital Solution For The Triple Star WDS 18253+4846 | |
| dc.type | text |