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Rotation in [C II]-emitting gas in two galaxies at a redshift of 6.8
Indexado
WoS WOS:000419794800030
Scopus SCOPUS_ID:85040455883
DOI 10.1038/NATURE24631
Año 2018
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



The earliest galaxies are thought to have emerged during the first billion years of cosmic history, initiating the ionization of the neutral hydrogen that pervaded the Universe at this time. Studying this 'epoch of reionization' involves looking for the spectral signatures of ancient galaxies that are, owing to the expansion of the Universe, now very distant from Earth and therefore exhibit large redshifts. However, finding these spectral fingerprints is challenging. One spectral characteristic of ancient and distant galaxies is strong hydrogen-emission lines (known as Lyman-alpha lines), but the neutral intergalactic medium that was present early in the epoch of reionization scatters such Lyman-alpha photons. Another potential spectral identifier is the line at wavelength 157.4 micrometres of the singly ionized state of carbon (the [C II] lambda = 157.74 mu m line), which signifies cooling gas and is expected to have been bright in the early Universe. However, so far Lyman-alpha-emitting galaxies from the epoch of reionization have demonstrated much fainter [C II] luminosities than would be expected from local scaling relations1-5, and searches for the [C II] line in sources without Lyman-a emission but with photometric redshifts greater than 6 (corresponding to the first billion years of the Universe) have been unsuccessful. Here we identify [C II]. = 157.74 mu m emission from two sources that we selected as high-redshift candidates on the basis of near-infrared photometry; we confirm that these sources are two galaxies at redshifts of z = 6.8540 +/- 0.0003 and z = 6.8076 +/- 0.0002. Notably, the luminosity of the [C II] line from these galaxies is higher than that found previously in star-forming galaxies with redshifts greater than 6.5. The luminous and extended [C II] lines reveal clear velocity gradients that, if interpreted as rotation, would indicate that these galaxies have similar dynamic properties to the turbulent yet rotation-dominated disks that have been observed in Ha-emitting galaxies two billion years later, at 'cosmic noon'.

Revista



Revista ISSN
Nature 0028-0836

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Disciplinas de Investigación



WOS
Multidisciplinary Sciences
Scopus
Sin Disciplinas
SciELO
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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Smit, Renske Mujer UNIV CAMBRIDGE - Reino Unido
Department of Physics - Reino Unido
University of Cambridge - Reino Unido
2 Bouwens, Richard Hombre Leiden Univ - Países Bajos
Leiden Observatory Research Institute - Países Bajos
Sterrewacht Leiden - Países Bajos
3 Carniani, Stefano Hombre UNIV CAMBRIDGE - Reino Unido
Department of Physics - Reino Unido
University of Cambridge - Reino Unido
4 Groves, B. Hombre Univ Geneva - Suiza
Université de Genève - Suiza
Faculty of Science - Suiza
5 Labbe, I. - Leiden Univ - Países Bajos
Leiden Observatory Research Institute - Países Bajos
Sterrewacht Leiden - Países Bajos
6 Illingworth, Garth Hombre Univ Calif Santa Cruz - Estados Unidos
University of California, Santa Cruz - Estados Unidos
Lick Observatory - Estados Unidos
7 van der Werf, Paul P. Hombre Leiden Univ - Países Bajos
Leiden Observatory Research Institute - Países Bajos
Sterrewacht Leiden - Países Bajos
8 Bradley, L. D. Hombre Space Telescope Sci Inst - Estados Unidos
STScI - Estados Unidos
Space Telescope Science Institute - Estados Unidos
9 Gonzalez, Vicente A. Hombre Universidad de Chile - Chile
Centro de Excelencia en Astrofísica y Tecnologías Afines - Chile
CATA - Chile
10 Hodge, Jacqueline Mujer Leiden Univ - Países Bajos
Leiden Observatory Research Institute - Países Bajos
Sterrewacht Leiden - Países Bajos
11 Holwerda, Benne W. - UNIV LOUISVILLE - Estados Unidos
University of Louisville - Estados Unidos
12 Maiolino, R. Hombre UNIV CAMBRIDGE - Reino Unido
Department of Physics - Reino Unido
University of Cambridge - Reino Unido
13 Zheng, Wei - Johns Hopkins Univ - Estados Unidos
Johns Hopkins University - Estados Unidos

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 3.9 %
Citas No-identificadas: 96.1 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 3.9 %
Citas No-identificadas: 96.1 %

Financiamiento



Fuente
National Science Foundation
European Research Council
National Research Council
Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council
Academia Sinica
Nederlandse Organisatie voor Wetenschappelijk Onderzoek
Korea Astronomy and Space Science Institute
National Institutes of Natural Sciences
Netherlands Organisation for Scientific Research (NWO)
Horizon 2020 Framework Programme
ERC Advanced Grant
National Institute of Natural Sciences
National Security Council
Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
Academia Sinica Institute

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Agradecimientos



Agradecimiento
This paper makes use of the following ALMA data: ADS/JAO.ALMA#2015.1.01111.S (http://almascience.org/aq?project_code=2015.1.01111.S). ALMA is a partnership of the European Southern Observatory (ESO, UK), the National Science Foundation (NSF, USA) and the National Institute of Natural Sciences (NINS, Japan), together with the National Research Council (NRC, Canada), the National Security Council (NSC) and Academia Sinica Institute of Astronomy and Astrophysics (ASIAA, Taiwan), and the Korea Astronomy and Space Science Institute (KASI, South Korea), in cooperation with Chile. The Joint ALMA Observatory is operated by ESO, Associated Universities Inc. (AUI)/National Radio Astronomy Observatory (NRAO), and the National Astronomical Observatory of Japan (NAOJ). This work is part of a Rubicon programme, 'A multi-wavelength view of the first galaxies', with project number 680-50-1518, which is financed by the Netherlands Organisation for Scientific Research (NWO). R.M. and S.C. acknowledge ERC Advanced Grant 695671 'QUENCH' and support by the Science and Technology Facilities Council (STFC).
Acknowledgements This paper makes use of the following ALMA data: ADS/JAO.ALMA#2015.1.01111.S (http://almascience.org/aq?project_ code=2015.1.01111.S). ALMA is a partnership of the European Southern Observatory (ESO, UK), the National Science Foundation (NSF, USA) and the National Institute of Natural Sciences (NINS, Japan), together with the National Research Council (NRC, Canada), the National Security Council (NSC) and Academia Sinica Institute of Astronomy and Astrophysics (ASIAA, Taiwan), and the Korea Astronomy and Space Science Institute (KASI, South Korea), in cooperation with Chile. The Joint ALMA Observatory is operated by ESO, Associated Universities Inc. (AUI)/National Radio Astronomy Observatory (NRAO), and the National Astronomical Observatory of Japan (NAOJ). This work is part of a Rubicon programme, ‘A multi-wavelength view of the first galaxies’, with project number 680-50-1518, which is financed by the Netherlands Organisation for Scientific Research (NWO). R.M. and S.C. acknowledge ERC Advanced Grant 695671 ‘QUENCH’ and support by the Science and Technology Facilities Council (STFC).

Muestra la fuente de financiamiento declarada en la publicación.