Unique sextuple system: 65 Ursae Majoris
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F12%3A10128494" target="_blank" >RIV/00216208:11320/12:10128494 - isvavai.cz</a>
Alternative codes found
RIV/67985815:_____/12:00388575
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201219134" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201219134</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201219134" target="_blank" >10.1051/0004-6361/201219134</a>
Alternative languages
Result language
angličtina
Original language name
Unique sextuple system: 65 Ursae Majoris
Original language description
We find that the system contains one more component, hence we tread it as a sextuple hierarchical system. The most inner pair of components consists of an eclipsing binary orbiting around a barycenter on a circular orbit, both components being almost identical of spectral type about A7. This pair orbits on an eccentric orbit around a barycenter, and the third component orbits with a period of about 640 days. This motion is reflected in the period variation in the minima times of the eclipsing pair, as well as in the radial velocities of the primary, secondary, and tertiary components. Moreover, this system orbits around a barycenter with the distant component resolved interferometrically, whose period is of about 118 years. Two more distant components(4 '' and 63 '') are also probably gravitationally bound to the system. The nodal period of the eclipsing-pair orbit is on the order of only a few centuries, which makes this system even more interesting for a future prospective detection
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GAP209%2F10%2F0715" target="_blank" >GAP209/10/0715: Accurate physical properties of hot stars based on binary and multiple star studies</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomy and Astrophysics
ISSN
0004-6361
e-ISSN
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Volume of the periodical
542
Issue of the periodical within the volume
červen
Country of publishing house
DE - GERMANY
Number of pages
6
Pages from-to
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UT code for WoS article
000305803300140
EID of the result in the Scopus database
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