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Witnessing globular cluster formation at z ∼ 3–10 with JWST and ELT

Published online by Cambridge University Press:  04 June 2020

Alvio Renzini Open the ORCID record for Alvio Renzini [Opens in a new window]
Alvio Renzini*
Affiliation:
INAF – Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, 35122, Padova, Italy email: alvio.renzini@inaf.it
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Abstract

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The opportunities offered by JWST and the ELT for the detection and study of forming/just formed globular clusters at high redshifts are illustrated, also alluding at the unique insight we may get on the very early stages of galaxy formation.

Keywords

globular clusters: generalgalaxies: high-redshiftgalaxies: evolutiongalaxies: formationgalaxies: star clusters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S352: Uncovering Early Galaxy Evolution in the ALMA and JWST Era , June 2019 , pp. 33 - 37
Copyright
© International Astronomical Union 2020

References

Bouwens, R. J., Illingworth, G. D., Oesch, P. A., Atek, H., Lam, D., & Stefanon, M. 2017, ApJ, 843, 4110.3847/1538-4357/aa74e4CrossRefGoogle Scholar
Bouwens, R. J., Illingworth, G. D., Oesch, P. A., Labbé, I.et al. 2018, 2018]boylan18Google Scholar
Boylan-Kolchin, M. 2018, MNRAS, 479, 332CrossRefGoogle Scholar
Carlberg, R. G. 2002, ApJ, 573, 6010.1086/340500CrossRefGoogle Scholar
Davies, R.et al. 2016, SPIE.9908E.1ZGoogle Scholar
Elmegreen, B. G. 2017, ApJ, 836, 8010.3847/1538-4357/836/1/80CrossRefGoogle Scholar
Hammer, F.et al. 2016, SPIE.9908E.24Google Scholar
Harris, W. E.et al. 2014, ApJ, 797, 12810.1088/0004-637X/797/2/128CrossRefGoogle Scholar
Katz, H. & Ricotti, M. 2013, MNRAS, 432, 325010.1093/mnras/stt676CrossRefGoogle Scholar
Katz, H. & Ricotti, M. 2014, MNRAS, 444, 237710.1093/mnras/stu1489CrossRefGoogle Scholar
Leaman, R., VandenBerg, D. A., & Mendel, J. T. 2013, MNRAS, 436, 12210.1093/mnras/stt1540CrossRefGoogle Scholar
Madau, P. & Dickinson, M. 2014, ARAA, 52, 41510.1146/annurev-astro-081811-125615CrossRefGoogle Scholar
Pozzetti, L., Maraston, C., & Renzini, A. 2019, MNRAS, 485, 586110.1093/mnras/stz785CrossRefGoogle Scholar
Ricotti, M. 2002, MNRAS, 336, L3310.1046/j.1365-8711.2002.05990.xCrossRefGoogle Scholar
Renzini, A. 2017, MNRAS, 469, L6310.1093/mnrasl/slx057CrossRefGoogle Scholar
Schraerer, D. & Charbonnel, C. 2011, MNRAS, 413, 2297CrossRefGoogle Scholar
Thatte, N. A.et al. 2016, SPIE.9908E.1XGoogle Scholar
Trenti, M., Padoan, P., & Jimenez, R. 2015, ApJ, 808, L35CrossRefGoogle Scholar
Vanzella, E.et al. 2016, ApJ, 821, L.27CrossRefGoogle Scholar
Vanzella, E.et al. 2017a, MNRAS, 467, 430410.1093/mnras/stx351CrossRefGoogle Scholar
Vanzella, E.et al. 2017b, MNRAS, 465, 380310.1093/mnras/stw2442CrossRefGoogle Scholar
Vanzella, E.et al. 2019, MNRAS, 483, 361810.1093/mnras/sty3311CrossRefGoogle Scholar
Zick, T. O., Weisz, D. R., & Boylan-Kolchin, M. 2018, MNRAS, 477, 48010.1093/mnras/sty662CrossRefGoogle Scholar