Looking deep into the Rosette Nebula's heart: the (sub)stellar content of the massive young cluster NGC 2244

As part of the ongoing effort to characterize the low-mass (sub)stellar population in a sample of massive young clusters, we have targeted the ~2 Myr old cluster NGC 2244. The distance to NGC 2244 from Gaia DR2 parallaxes is 1.59 kpc, with errors of 1% (statistical) and 11% (systematic). We used the...

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Veröffentlicht in:	arXiv.org 2019-07
Hauptverfasser:	Muzic, Koraljka, Scholz, Alexander, Karla Pena Ramirez, Jayawardhana, Ray, Schoedel, Rainer, Geers, Vincent C, Cieza, Lucas A, Bayo, Amelia
Format:	Artikel
Sprache:	eng
Schlagworte:	Brown dwarf stars Clusters Color-magnitude diagram Filaments Infrared cameras Initial mass function Low mass stars Massive stars Nebulae Physics - Astrophysics of Galaxies Physics - Solar and Stellar Astrophysics Population (statistical) Star formation
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