RT Journal Article
T1 20 Orbits of binaries based on soar speckle observations
T2 Twenty Orbits of binaries based on soar speckle observations
A1 Gómez Crespo, Jorge
A1 Docobo, José Ángel
A1 Campo Díaz, Pedro Pablo
A1 Andrade Baliño, Manuel
A1 Méndez, René A.
A1 Costa, Edgardo
K1 Techniques
K1 High angular resolution
K1 Astrometry
K1 Binaries
K1 Visual
K1 Stars
K1 Fundamental parameters
AB New observational data obtained during the 2018, 2019, and 2020 speckle runs with the 4.1-m Southern Astrophysical Research (SOAR) telescope located at Cerro Pachón (Chile) allowed us to recalculate the orbits of the visual binaries: WDS 00277-1625 (YR 1 Aa,Ab), WDS 00462-2214 (RST4155), WDS 03124-4425 (JC 8), WDS 07427-3510 (HDS 1091), WDS 10093+2020 (A2145), WDS 10116+1321 (HU 874 AB), WDS 10217-0946 (BU 25), WDS 11585-2350 (RST 3767 AB), WDS 13117-2633 (FIN 305), WDS 13305+0729 (A 1789), and WDS 16458-0046 (A1141). In addition, we present the first orbits calculated for the following binaries: WDS 07303-5657 (FIN 105), WDS 09110-1929 (I 824), WDS 12111-5302 (HU 1604), WDS 14592-4206 (HDS 2116 Aa,Ab), WDS 15157-2736 (BU 350), WDS 15493+0503 (A 1126), WDS 16402-2800 (VOU 44 AB), and WDS 18126+1224 (HDS 2570). All of them are placed below Dec. + 21° and the majority are main-sequence stars. Except in cases with giant components or close triple systems, the ANAPAR method was used in order to obtain precise dynamical parallaxes and individual masses. These parallaxes were compared with those obtained by Gaia and/or Hipparcos satellites. In the case of FIN 305, we present two different orbital solutions. Also, using the dynamical parallaxes given by these orbits, we have been able to calculate the luminosity of these systems. Said luminosities allow us to indicate an approximate age for the components of these systems, situating them within the Hertzsprung-Russell (HR) diagram. In addition, a commentary for each binary about the physical and dynamical properties of the studied binaries has been included
PB Oxford University Press
SN 0035-8711
YR 2021
FD 2021
LK http://hdl.handle.net/10347/28871
UL http://hdl.handle.net/10347/28871
LA eng
NO Jorge Gómez, José A Docobo, Pedro P Campo, Manuel Andrade, Rene A Mendez., Edgardo Costa, 20 Orbits of binaries based on soar speckle observations, Monthly Notices of the Royal Astronomical Society, Volume 509, Issue 3, January 2022, Pages 4229–4245, https://doi.org/10.1093/mnras/stab2633
NO We are very grateful for the continuous support of the Chilean Telescope Allocation Committee: http://www.das.uchile.cl/das_cntac.html under programs CN2018A-1, CN2019A-2, CN2019B-13, and CN2020A-19 and 2020B-10. This paper was supported by the ‘Xunta de Galicia’ (Spain), under the ED431B 2020/38 grant. RAM and EC acknowledge support from ANID/FONDECYT grant 1190038
DS Minerva
RD 29 abr 2026