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| DOI | 10.1093/MNRAS/STAD2065 | ||||
| Año | 2023 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Stellar hierarchical systems of high order containing more than three stars are rare and fascinating objects; their discovery and study highlight still unknown aspects of star formation and early evolution. We matched eclipsing binaries discovered by Transiting Exoplanet Survey Satellite with a Gaia catalogue of wide binaries and selected candidate quadruple (or higher order) systems based on excessive astrometric noise. A subset of 192 southern candidates located within 500 pc was observed by speckle interferometry, and we resolved for the first time 50 close pairs, confirming their high-order (from four to five components) multiplicity. These observations are reported, and some remarkable hierarchical systems are discussed.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Powell, Brian P. | Hombre |
NASA Goddard Space Flight Ctr - Estados Unidos
NASA Goddard Space Flight Center - Estados Unidos |
| 2 | Kostov, Veselin | Hombre |
NASA Goddard Space Flight Ctr - Estados Unidos
SETI Inst - Estados Unidos SETI Institute - Estados Unidos NASA Goddard Space Flight Center - Estados Unidos |
| 3 | Tokovinin, Andrei | Hombre |
Cerro Tololo Interamer Observ NSFs NOIRLab - Chile
Cerro Tololo Inter American Observatory - Chile |
| Fuente |
|---|
| National Science Foundation |
| National Aeronautics and Space Administration |
| NASA's Science Mission directorate |
| NASA Center for Climate Simulation |
| Science Mission Directorate |
| NSF's NOIRLab |
| NASA High-End Computing (HEC) Program through the NASA Center for Climate Simulation (NCCS) at Goddard Space Flight Center |
| Agradecimiento |
|---|
| Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Center for Climate Simulation (NCCS) at Goddard Space Flight Center.This paper includes data collected by the TESS mission, which are publicly available from the Mikulski Archive for Space Telescopes (MAST). Funding for the TESS mission was provided by NASA's Science Mission Directorate.This research was partially funded by the NSF's NOIRLab. This work used the SIMBAD service operated by Centre des Donnees Stellaires (Strasbourg, France), bibliographic references from the Astrophysics Data System maintained by SAO/NASA, and the Washington Double Star Catalog maintained at USNO.This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. |
| This paper includes data collected by the TESS mission, which are publicly available from the Mikulski Archive for Space Telescopes (MAST). Funding for the TESS mission was provided by NASA’s Science Mission Directorate. |
| Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Center for Climate Simulation (NCCS) at Goddard Space Flight Center. |
| This paper includes data collected by the TESS mission, which are publicly available from the Mikulski Archive for Space Telescopes (MAST). Funding for the TESS mission was provided by NASA’s Science Mission Directorate. |