JWST/NIRCam detections of dusty subsolar-mass young stellar objects in the Small Magellanic Cloud
Author:
Funder
STFC Webb Fellowship
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
https://www.nature.com/articles/s41550-023-01945-7.pdf
Reference57 articles.
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2. Bouret, J. C. et al. Quantitative spectroscopy of O stars at low metallicity: O dwarfs in NGC 346. Astrophys. J. 595, 1182–1205 (2003).
3. Peimbert, M., Peimbert, A. & Ruiz, M. T. The chemical composition of the Small Magellanic Cloud H II Region NGC 346 and the primordial helium abundance. Astrophys. J. 541, 688–700 (2000).
4. Madau, P. & Dickinson, M. Cosmic star-formation history. Annu. Rev. Astron. Astrophys. 52, 415–486 (2014).
5. Dimaratos, A., Cormier, D., Bigiel, F. & Madden, S. C. Modeling the physical properties in the ISM of the low-metallicity galaxy NGC 4214. Astron. Astrophys. 580, A135 (2015).
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