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High-redshift starbursts as progenitors of massive galaxies

Published online by Cambridge University Press:  29 March 2021

Carlos Gómez-Guijarro Open the ORCID record for Carlos Gómez-Guijarro [Opens in a new window]
Carlos Gómez-Guijarro*
Affiliation:
AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, France email: carlos.gomezguijarro@cea.fr
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Abstract

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Starbursting dust-rich galaxies are capable of assembling large amounts of stellar mass very quickly. They have been proposed as progenitors of the population of compact massive quiescent galaxies at z ˜ 2. To test this connection, we present a detailed spatially-resolved study of the stars, dust, and stellar mass in a sample of six submillimeter-bright starburst galaxies at z ˜ 4.5. We found that the systems are undergoing minor mergers and the bulk star formation is located in extremely compact regions. On the other hand, optically-compact star forming galaxies have also been proposed as immediate progenitors of compact massive quiescent galaxies. Were they formed in slow secular processes or in rapid merger-driven starbursts? We explored the location of galaxies with respect to star-forming and structural relations and study the burstiness of star formation. Our results suggest that compact star-forming galaxies could be starbursts winding down and eventually becoming quiescent.

Keywords

galaxies: bulgesgalaxies: evolutiongalaxies: formationgalaxies: fundamental parametersgalaxies: high-redshiftgalaxies: interactionsgalaxies: ISMgalaxies: starburst
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 22 - 26
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

References

Barro, G., Faber, S. M., Pérez-González, P. G., et al. 2013, ApJ, 765, 104 CrossRefGoogle Scholar
Barro, G., Faber, S. M., Koo, D. C., et al. 2017, ApJ, 840, 47 CrossRefGoogle Scholar
Belli, S., Newman, A. B., & Ellis, R. S. 2017, ApJ, 834, 18 CrossRefGoogle Scholar
Bezanson, R., van Dokkum, P.G., Tal, T., et al. 2009, ApJ (Letters), 697, 1290 Google Scholar
Bressan, A., Silva, L., Granato, G. L., et al. 2002, A&A, 392, 377 Google Scholar
Casey, C. M., Narayanan, D. & Cooray, A. 2014, PhR, 541, 45 Google Scholar
Elbaz, D., Daddi, E., Le Borgne, D., et al. 2007, A&A, 468, 33 Google Scholar
Elbaz, D., Leiton, R., Nagar, N., et al. 2018, A&A, 616, A110 Google Scholar
Gómez-Guijarro, C., Toft, S., Karim, A., et al. 2018, ApJ, 856, 121 CrossRefGoogle Scholar
Gómez-Guijarro, C., Magdis, G. E., Valentino, F., et al. 2019, ApJ, 886, 88 CrossRefGoogle Scholar
Hodge, J. A., Swinbank, A. M., Simpson, J. M., et al. 2016, ApJ, 833, 103 CrossRefGoogle Scholar
Jones, G. C., Carilli, C. L., Shao, Y., et al. 2017, ApJ, 850, 180 CrossRefGoogle Scholar
Kauffmann, G., Heckman, T. M., Tremonti, C., et al. 2003, MNRAS, 346, 1055 CrossRefGoogle Scholar
Krogager, J. K., Zirm, A. W., Toft, S., et al. 2014, ApJ, 797, 17 CrossRefGoogle Scholar
Meurer, G. R., Heckman, T. M., Calzetti, D., et al. 1999, ApJ, 521, 64 CrossRefGoogle Scholar
Newman, A. B., Ellis, R. S., Bundy, K., et al. 2012, ApJ, 746, 162 CrossRefGoogle Scholar
Newman, A. B., Belli, S., Ellis, R. S., et al. 2015, ApJ (Letters), 813, L7 Google Scholar
Noeske, K. G., Weiner, B. J., Faber, S. M., et al. 2007, ApJ (Letters), 660, L43 Google Scholar
Lee, B., Giavalisco, M., Whitaker, K., et al. 2018, ApJ, 853, 131 CrossRefGoogle Scholar
Tadaki, K., Iono, D., Yun, M., et al. 2020, ApJ, 889, 141 CrossRefGoogle Scholar
Thomson, A. P., Ivison, R. J., Simpson, J. M., et al. 2014, MNRAS, 442, 577 CrossRefGoogle Scholar
Toft, S., van Dokkum, P., Franx, M., et al. 2007, ApJ, 671, 285 CrossRefGoogle Scholar
Toft, S., Smolčić, V., Magnelli, B., et al. 2014, ApJ, 782, 68 CrossRefGoogle Scholar
Toft, S., Zabl, J., Richard, J., et al. 2017, Nature, 546, 510 CrossRefGoogle Scholar
van Dokkum, P. G., Franx, M., Kriek, M., et al. 2008, ApJL (Letters), 677, L5 Google Scholar
van Dokkum, P. G., Nelson, E. J., Franx, M., et al. 2015, ApJ, 813, 23 CrossRefGoogle Scholar
van de Sande, J., Kriek, M., Franx, M., et al. 2013, ApJ, 771, 85 CrossRefGoogle Scholar
van der Wel, A., Franx, M., van Dokkum, P. G., et al. 2014, ApJ, 788, 28 CrossRefGoogle Scholar