Near-infrared Stellar Populations in the Metal-poor, Dwarf Irregular Galaxies Sextans A and Leo A

Autor: Margaret Meixner, Olivia Jones, Helen Meskhidze, Martha L. Boyer, Matthew T. Maclay, Iain McDonald
Rok vydání: 2018
Předmět:
Zdroj: The Astrophysical Journal
Jones, O C, Maclay, M T, Boyer, M L, Meixner, M, McDonald, I & Meskhidze, H 2018, ' Near-infrared Stellar Populations in the Metal-poor, Dwarf Irregular Galaxies Sextans A and Leo A ', Astrophysical Journal, vol. 854, no. 2, 117 . https://doi.org/10.3847/1538-4357/aaa542
ISSN: 1538-4357
1538-3881
0004-6361
0004-637X
0067-0049
0002-7537
DOI: 10.3847/1538-4357/aaa542
Popis: We present JHK$_{s}$ observations of the metal-poor ([Fe/H] $10^{-11}$ $M_\odot \,{\rm yr}^{-1}$, confirming that metal-poor stars can form substantial amounts of dust. We also find tentative evidence for oxygen-rich dust formation at low metallicity, contradicting previous models that suggest oxygen-rich dust production is inhibited in metal-poor environments. The total rates of dust injection into the interstellar medium of Leo A and Sextans A are (8.2 $\pm$ 1.8) $\times 10^{-9}$ $M_\odot \,{\rm yr}^{-1}$ and (6.2 $\pm$ 0.2) $\times 10^{-7}$ $M_\odot \,{\rm yr}^{-1}$, respectively. The majority of this dust is produced by a few very dusty evolved stars, and does not vary strongly with metallicity.
Comment: 21 pages, 11 figures, 10 tables; accepted for publication in ApJ
Databáze: OpenAIRE