Beyond the Local Volume. II. Population Scaleheights and Ages of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields

Ultracool dwarfs represent a significant proportion of stars in the Milky Way,and deep samples of these sources have the potential to constrain the formation history and evolution of low-mass objects in the Galaxy. Until recently, spectral samples have been limited to the local volume (d

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Bibliographische Detailangaben
Veröffentlicht in:	arXiv.org 2022-08
Hauptverfasser:	Aganze, Christian, Burgasser, Adam J, Malkan, Matthew A, Theissen, Christopher A, Tejada Arevalo, Roberto A, Hsu, Chih-Chun, Daniella C Bardalez Gagliuffi, Ryan, Russell E, Holwerda, Benne W
Format:	Artikel
Sprache:	eng
Schlagworte:	Age Constraint modelling Hubble Space Telescope Infrared spectroscopy Infrared telescopes Luminosity Physics - Astrophysics of Galaxies Physics - Solar and Stellar Astrophysics Population Red dwarf stars Simulation Space telescopes Star & galaxy formation Star formation Three dimensional models
Online-Zugang:	Volltext
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Beschreibung
Zusammenfassung:	Ultracool dwarfs represent a significant proportion of stars in the Milky Way,and deep samples of these sources have the potential to constrain the formation history and evolution of low-mass objects in the Galaxy. Until recently, spectral samples have been limited to the local volume (d
ISSN:	2331-8422
DOI:	10.48550/arxiv.2204.07621