Wide [Sigma] Orionis binaries resolved by UKIDSS
In spite of its importance for the study of star formation at all mass domains, the nearby young σ Orionis cluster still lacks a comprehensive survey for multiplicity. We try to fill that observational gap by looking for wide resolved binaries with angular separations between 0.4 and 4.0 arcsec. We...
Gespeichert in:
| Hauptverfasser: | , , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018
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| In: |
Astronomische Nachrichten
Year: 2017, Jahrgang: 339, Heft: 1, Pages: 60-71 |
| ISSN: | 1521-3994 |
| DOI: | 10.1002/asna.201713314 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1002/asna.201713314 Verlag, lizenzpflichtig, Volltext: https://onlinelibrary.wiley.com/doi/abs/10.1002/asna.201713314 
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| Verfasserangaben: | J.A. Caballero, I. Novalbos, T. Tobal, F.X. Miret |
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A TGAS/Gaia DR1 parallactic distance to the [sigma] Orionis cluster
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