Cosmicflows-3: The South Pole Wall
International audience Velocity and density field reconstructions of the volume of the universe within 0.05c derived from the Cosmicflows-3 catalog of galaxy distances has revealed the presence of a filamentary structure extending across ∼0.11c. The structure, at a characteristic redshift of 12,000...
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ftanrparis:oai:HAL:hal-02905192v1 2024-09-30T14:43:40+00:00 Cosmicflows-3: The South Pole Wall Pomarède, Daniel Tully, R. Brent Graziani, Romain Courtois, Hélène M. Hoffman, Yehuda Lezmy, Jérémy Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU) Université Paris-Saclay-Direction de Recherche Fondamentale (CEA) (DRF (CEA)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA) Laboratoire de Physique de Clermont (LPC) Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne 2017-2020 (UCA 2017-2020 )-Centre National de la Recherche Scientifique (CNRS) Institut de Physique des 2 Infinis de Lyon (IP2I Lyon) Université Claude Bernard Lyon 1 (UCBL) Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) ANR-16-IDEX-0005,IDEXLYON,IDEXLYON(2016) 2020 https://hal.science/hal-02905192 https://doi.org/10.3847/1538-4357/ab9952 en eng HAL CCSD American Astronomical Society info:eu-repo/semantics/altIdentifier/arxiv/2007.04414 info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ab9952 hal-02905192 https://hal.science/hal-02905192 ARXIV: 2007.04414 doi:10.3847/1538-4357/ab9952 INSPIRE: 1806072 ISSN: 0004-637X EISSN: 1538-4357 The Astrophysical Journal https://hal.science/hal-02905192 The Astrophysical Journal, 2020, 897 (2), pp.133. ⟨10.3847/1538-4357/ab9952⟩ [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/article Journal articles 2020 ftanrparis https://doi.org/10.3847/1538-4357/ab9952 2024-09-05T00:06:58Z International audience Velocity and density field reconstructions of the volume of the universe within 0.05c derived from the Cosmicflows-3 catalog of galaxy distances has revealed the presence of a filamentary structure extending across ∼0.11c. The structure, at a characteristic redshift of 12,000 km s−1, has a density peak coincident with the celestial South Pole. This structure, the largest contiguous feature in the local volume and comparable to the Sloan Great Wall at half the distance, is given the name the South Pole Wall. Article in Journal/Newspaper South pole Portail HAL-ANR (Agence Nationale de la Recherche) South Pole The Astrophysical Journal 897 2 133 |
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Portail HAL-ANR (Agence Nationale de la Recherche) |
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English |
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[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
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[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Pomarède, Daniel Tully, R. Brent Graziani, Romain Courtois, Hélène M. Hoffman, Yehuda Lezmy, Jérémy Cosmicflows-3: The South Pole Wall |
topic_facet |
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
description |
International audience Velocity and density field reconstructions of the volume of the universe within 0.05c derived from the Cosmicflows-3 catalog of galaxy distances has revealed the presence of a filamentary structure extending across ∼0.11c. The structure, at a characteristic redshift of 12,000 km s−1, has a density peak coincident with the celestial South Pole. This structure, the largest contiguous feature in the local volume and comparable to the Sloan Great Wall at half the distance, is given the name the South Pole Wall. |
author2 |
Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU) Université Paris-Saclay-Direction de Recherche Fondamentale (CEA) (DRF (CEA)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA) Laboratoire de Physique de Clermont (LPC) Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne 2017-2020 (UCA 2017-2020 )-Centre National de la Recherche Scientifique (CNRS) Institut de Physique des 2 Infinis de Lyon (IP2I Lyon) Université Claude Bernard Lyon 1 (UCBL) Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) ANR-16-IDEX-0005,IDEXLYON,IDEXLYON(2016) |
format |
Article in Journal/Newspaper |
author |
Pomarède, Daniel Tully, R. Brent Graziani, Romain Courtois, Hélène M. Hoffman, Yehuda Lezmy, Jérémy |
author_facet |
Pomarède, Daniel Tully, R. Brent Graziani, Romain Courtois, Hélène M. Hoffman, Yehuda Lezmy, Jérémy |
author_sort |
Pomarède, Daniel |
title |
Cosmicflows-3: The South Pole Wall |
title_short |
Cosmicflows-3: The South Pole Wall |
title_full |
Cosmicflows-3: The South Pole Wall |
title_fullStr |
Cosmicflows-3: The South Pole Wall |
title_full_unstemmed |
Cosmicflows-3: The South Pole Wall |
title_sort |
cosmicflows-3: the south pole wall |
publisher |
HAL CCSD |
publishDate |
2020 |
url |
https://hal.science/hal-02905192 https://doi.org/10.3847/1538-4357/ab9952 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
ISSN: 0004-637X EISSN: 1538-4357 The Astrophysical Journal https://hal.science/hal-02905192 The Astrophysical Journal, 2020, 897 (2), pp.133. ⟨10.3847/1538-4357/ab9952⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/2007.04414 info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ab9952 hal-02905192 https://hal.science/hal-02905192 ARXIV: 2007.04414 doi:10.3847/1538-4357/ab9952 INSPIRE: 1806072 |
op_doi |
https://doi.org/10.3847/1538-4357/ab9952 |
container_title |
The Astrophysical Journal |
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897 |
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2 |
container_start_page |
133 |
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1811645373291167744 |