Fabiola Campos, Ingrid Domingos Pelisoli, Sebastian Kamann, T. -O. Husser, S. Dreizler, A. Bellini, E. L. Robinson, Domenico Nardiello, G. Piotto, S. O. Kepler, A. G. Istrate, D. E. Winget, M. H. Montgomery, A. Dotter
- We use Hubble Space Telescope multicolour photometry of the globular cluster 47 Tucanae to uncover a population of 24 objects with no previous classification that are outliers from the single-star model tracks in the colour-magnitude diagram and yet are likely cluster members. By comparing those sources with evolutionary models and X-ray source catalogues, we were able to show that the majority of those sources are likely binary systems that do not have any X-ray source detected nearby, most possibly formed by a white dwarf and a main-sequence star and a small number of possible double-degenerate systems.
Metadaten| Verfasserangaben: | Fabiola CamposORCiD, Ingrid Domingos PelisoliORCiD, Sebastian KamannORCiD, T. -O. Husser, S. Dreizler, A. Bellini, E. L. Robinson, Domenico NardielloORCiD, G. Piotto, S. O. KeplerORCiD, A. G. Istrate, D. E. Winget, M. H. Montgomery, A. Dotter |
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| DOI: | https://doi.org/10.1093/mnras/sty2591 |
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| ISSN: | 0035-8711 |
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| ISSN: | 1365-2966 |
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| Titel des übergeordneten Werks (Englisch): | Monthly notices of the Royal Astronomical Society |
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| Untertitel (Englisch): | multicolour photometry guiding the search for evolved binary systems in the globular cluster 47 Tucanae |
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| Verlag: | Oxford Univ. Press |
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| Verlagsort: | Oxford |
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| Publikationstyp: | Wissenschaftlicher Artikel |
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| Sprache: | Englisch |
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| Datum der Erstveröffentlichung: | 20.09.2018 |
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| Erscheinungsjahr: | 2018 |
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| Datum der Freischaltung: | 15.06.2021 |
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| Freies Schlagwort / Tag: | Hertzsprung-Russell and colour-magnitude diagrams; binaries: general; globular clusters: individual: 47 Tuc; white dwarfs |
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| Band: | 481 |
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| Ausgabe: | 4 |
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| Seitenanzahl: | 13 |
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| Erste Seite: | 4397 |
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| Letzte Seite: | 4409 |
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| Fördernde Institution: | NASANational Aeronautics & Space Administration (NASA) [NAS 5-26555, NNX13AH43G]; NSFNational Science Foundation (NSF) [AST-1211616, AST 1707419, AST-1313280]; DFGGerman Research Foundation (DFG) [GE 2056-12-1]; CNPq-BrazilNational Council for Scientific and Technological Development (CNPq); European Research Council (Multi-Pop) [ERC-CoG-646928]; German Ministry for Education and Science (BMBF Verbundforschung) [05A14MGA, 05A17MGA, 05A14BAC, 05A17BAA]; German Research Foundation (DFG)German Research Foundation (DFG) [DR 281/35-1, KA 4537/2-1]; HST [AR-12845, GO-13297]; Universit a degli Studi di Padova Progetto di Ateneo [CPDA141214, BIRD178590]; INAF under the program PRIN-INAF2014; United States Department of EnergyUnited States Department of Energy (DOE) [DE-SC0010623]; Wooton Center for Astrophysical Plasma Properties under the United States Department of Energy [DE-FOA-0001634] |
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| Organisationseinheiten: | Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie |
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| DDC-Klassifikation: | 5 Naturwissenschaften und Mathematik / 52 Astronomie / 520 Astronomie und zugeordnete Wissenschaften |
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| Peer Review: | Referiert |
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| Publikationsweg: | Open Access / Bronze Open-Access |
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