HD 152246: a new high-mass triple system and its basic properties
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F14%3A10287024" target="_blank" >RIV/00216208:11320/14:10287024 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201424382" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201424382</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201424382" target="_blank" >10.1051/0004-6361/201424382</a>
Alternative languages
Result language
angličtina
Original language name
HD 152246: a new high-mass triple system and its basic properties
Original language description
Analyses of multi-epoch, high-resolution (R similar to 50 000) optical spectra of the O-type star HD 152246 (09 IV according to the most recent classification), complemented by a limited number of earlier published radial velocities, led to the finding that the object is a hierarchical triple system, where a close inner pair (Ba-Bb) with a slightly eccentric orbit (e = 0.11) and a period of 6.0049 revolves in a 470-day highly eccentric orbit (e = 0.865) with another massive and brighter component A. Themass ratio of the inner system must be low since we were unable to find any traces of the secondary spectrum. The mass ratio A/(Ba+Bb) is 0.89. The outer system has recently been resolved using long-baseline interferometry on three occasions. The interferometry confirms the spectroscopic results and specifies elements of the system. Our orbital solutions, including the combined radial-velocity and interferometric solution indicate an orbital inclination of the outer orbit of 112 and ste
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
Z - Vyzkumny zamer (s odkazem do CEZ)<br>S - Specificky vyzkum na vysokych skolach
Others
Publication year
2014
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
568
Issue of the periodical within the volume
srpen
Country of publishing house
FR - FRANCE
Number of pages
9
Pages from-to
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UT code for WoS article
000341185900131
EID of the result in the Scopus database
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