A TGAS/Gaia DR1 parallactic distance to the [sigma] Orionis cluster

With the new Tycho?Gaia Astrometric Solution (TGAS), I derive a new parallactic distance to the young σ Orionis open cluster, which is a cornerstone region for studying the formation and evolution of stars and substellar objects from tens of solar masses to a few Jupiter masses. I started with the l...

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Bibliographic Details
Main Author:	Caballero, José A. (Author)
Format:	Article (Journal)
Language:	English
Published:	18 April 2017
In:	Astronomische Nachrichten Year: 2017, Volume: 338, Issue: 5, Pages: 629-634
ISSN:	1521-3994
DOI:	10.1002/asna.201713312
Online Access:	Verlag, Volltext: http://dx.doi.org/10.1002/asna.201713312 Verlag, Volltext: https://onlinelibrary.wiley.com/doi/abs/10.1002/asna.201713312
Author Notes:	José A. Caballero

Wide [Sigma] Orionis binaries resolved by UKIDSS by Caballero, José A. (Author) , Novalbos, I. (Author) , Tobal, T. (Author) , Miret, F. X. (Author) ,

in: Astronomische Nachrichten, 339 (2018), 1, Seite 60-71

Article (Journal) Online Resource

A TGAS/Gaia DR1 parallactic distance to the [sigma] Orionis cluster

Wide [Sigma] Orionis binaries resolved by UKIDSS by Caballero, José A. (Author) , Novalbos, I. (Author) , Tobal, T. (Author) , Miret, F. X. (Author) ,

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