Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Marie Lou Gendron-Marsolais"'
Autor:
Benjamin Vigneron, Julie Hlavacek-Larrondo, Carter Lee Rhea, Marie-Lou Gendron-Marsolais, Jeremy Lim, Jake Reinheimer, Yuan Li, Laurent Drissen, Greg L. Bryan, Megan Donahue, Alastair Edge, Andrew Fabian, Stephen Hamer, Thomas Martin, Michael McDonald, Brian McNamara, Annabelle Richard-Lafferrière, Laurie Rousseau-Nepton, G. Mark Voit, Tracy Webb, Norbert Werner
Publikováno v:
The Astrophysical Journal, Vol 962, Iss 1, p 96 (2024)
We present new high-spectral-resolution observations ( R = λ /Δ λ = 7000) of the filamentary nebula surrounding NGC 1275, the central galaxy of the Perseus cluster. These observations have been obtained with SITELLE, an imaging Fourier transform s
Externí odkaz:
https://doaj.org/article/5b391d88c8d74f079de0cfed8ad5e4cb
Autor:
Congyao Zhang, Irina Zhuravleva, Marie-Lou Gendron-Marsolais, Eugene Churazov, Alexander A Schekochihin, William R Forman
Buoyant bubbles of relativistic plasma are essential for active galactic nucleus feedback in galaxy clusters, stirring and heating the intracluster medium (ICM). Observations suggest that these rising bubbles maintain their integrity and sharp edges
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb166d5290fdce69160e19157e5635df
http://arxiv.org/abs/2203.04259
http://arxiv.org/abs/2203.04259
Autor:
Haojie Hu, Yu Qiu, Marie-Lou Gendron-Marsolais, Tamara Bogdanović, Julie Hlavacek-Larrondo, Luis C. Ho, Kohei Inayoshi, Brian R. McNamara
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the origina
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::270e0eb11ae06059c96158bfa9a0294a
http://hdl.handle.net/10261/273209
http://hdl.handle.net/10261/273209
Autor:
Julie Hlavacek-Larrondo, Marie-Lou Gendron-Marsolais, A. Richard-Laferrière, Lawrence Rudnick, Emmet Golden-Marx, J. D. McBride, Charles L. H. Hull, Elke Roediger, Richard A. Perley, N. Arakawa, Andrew C. Fabian, R. J. van Weeren, Ralph P. Kraft
Publikováno v:
The Astrophysical Journal, 911(1)
We present new deep, high-resolution, 1.5 GHz observations of the prototypical nearby Perseus galaxy cluster from the Karl G. Jansky Very Large Array. We isolate for the first time the complete tail of radio emission of the bent-jet radio galaxy NGC
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e443a3d14020d95bc13ee1ec3431cab
http://arxiv.org/abs/2101.05305
http://arxiv.org/abs/2101.05305
Autor:
Israel Matute, C. Yang, Stergios Amarantidis, Tony Mroczkowski, Mark Lacy, David Rebolledo, Brian Mason, Hugo Messias, R. Kneissl, Evanthia Hatziminaoglou, Sonia Antón, Ricardo Demarco, Marie Lou Gendron-Marsolais, Edward B. Fomalont, Paulo C. Cortes, Pascale Hibon, Jose Afonso, Andrew M. Hopkins, Cristian Lopez, Sergio Martín
Radio-emitting jets might be one of the main ingredients shaping the evolution of massive galaxies in the Universe since early cosmic times. However, identifying early radio active galactic nuclei (AGN) and confirming this scenario has been hard to a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::68a1b3760d60393ec772edab075a4642
Autor:
R. J. van Weeren, Lawrence Rudnick, Marie-Lou Gendron-Marsolais, Jeremy S. Sanders, Katherine M. Blundell, Tracy E. Clarke, Julie Hlavacek-Larrondo, Biny Sebastian, Wendy Peters, Kristina Nyland, E. Sheldahl, Hubertus Intema, Andrew C. Fabian, Tony Mroczkowski
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 499(4), 5791-5805
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
We present the first high-resolution 230-470 MHz map of the Perseus cluster obtained with the Karl G. Jansky Very Large Array. The high dynamic range and resolution achieved has allowed the identification of previously-unknown structures in this near
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b0adc66b0cb8c242dfe0c37805d082a
http://hdl.handle.net/1887/3133810
http://hdl.handle.net/1887/3133810
Autor:
Myungkook J. Jee, Gillian Wilson, Kyle Finner, Michael McDonald, Jason Surace, A. Trudeau, Julie Hlavacek-Larrondo, Michael C. Cooper, Howard K. C. Yee, Helen Russell, Marie Lou Gendron-Marsolais, Adam Muzzin, F. Valin, N. Bonaventura, T. M. A. Webb, Andrew C. Fabian, M. Mezcua, Carter Rhea, Allison Noble, C. Lidman
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Hlavacek-Larrondo, J, Rhea, C L, Webb, T, McDonald, M, Muzzin, A, Wilson, G, Finner, K, Valin, F, Bonaventura, N, Cooper, M, Fabian, A C, Gendron-Marsolais, M-L, Jee, M J, Lidman, C, Mezcua, M, Noble, A, Russell, H R, Surace, J, Trudeau, A & Yee, H K C 2020, ' Evidence of Runaway Gas Cooling in the Absence of Supermassive Black Hole Feedback at the Epoch of Cluster Formation ', Astrophysical Journal Letters, vol. 898, no. 2, 50 . https://doi.org/10.3847/2041-8213/ab9ca5
instname
Hlavacek-Larrondo, J, Rhea, C L, Webb, T, McDonald, M, Muzzin, A, Wilson, G, Finner, K, Valin, F, Bonaventura, N, Cooper, M, Fabian, A C, Gendron-Marsolais, M-L, Jee, M J, Lidman, C, Mezcua, M, Noble, A, Russell, H R, Surace, J, Trudeau, A & Yee, H K C 2020, ' Evidence of Runaway Gas Cooling in the Absence of Supermassive Black Hole Feedback at the Epoch of Cluster Formation ', Astrophysical Journal Letters, vol. 898, no. 2, 50 . https://doi.org/10.3847/2041-8213/ab9ca5
arXiv:2007.15660v1
Cosmological simulations, as well as mounting evidence from observations, have shown that supermassive black holes play a fundamental role in regulating the formation of stars throughout cosmic time. This has been clearly demo
Cosmological simulations, as well as mounting evidence from observations, have shown that supermassive black holes play a fundamental role in regulating the formation of stars throughout cosmic time. This has been clearly demo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a38209ac1135dd8f6eea646572c0c1b7
https://resolver.caltech.edu/CaltechAUTHORS:20200803-122222162
https://resolver.caltech.edu/CaltechAUTHORS:20200803-122222162
Magnetic fields in the intracluster medium (ICM) affect the structure and the evolution of galaxy clusters. However, their properties are largely unknown, and measuring magnetic fields in galaxy clusters is challenging, especially on large-scales out
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c63e59d26becfd0a892a0aa3dfb24fae
Autor:
Ethan T. Vishniac, Lev Arzamasskiy, Irina Zhuravleva, Greg L. Bryan, Matteo Fossati, Alessandro Boselli, Eric Emsellem, Miao Li, Cassandra Lochhaas, Siyao Xu, Aurora Simionescu, Yong Zheng, Julie Hlavacek-Larrondo, Marie Lou Gendron-Marsolais, Eliot Quataert, Grant R. Tremblay, Marc Sarzi, Norman Murray, Yuan Li
Publikováno v:
Astrophys.J.Lett.
Astrophys.J.Lett., 2020, 889 (1), pp.L1. ⟨10.3847/2041-8213/ab65c7⟩
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2020, 889 (1), pp.L1. ⟨10.3847/2041-8213/ab65c7⟩
The Astrophysical journal letters, 2020, 889 (1), pp.L1. ⟨10.3847/2041-8213/ab65c7⟩
Astrophys.J.
Astrophys.J., 2020, 889 (1), pp.L1. ⟨10.3847/2041-8213/ab65c7⟩
The Astrophysical Journal
The Astrophysical Journal Letters, 889(1), L1
Astrophysical journal, 2020, Vol.889(1), pp.L1 [Peer Reviewed Journal]
Astrophys.J.Lett., 2020, 889 (1), pp.L1. ⟨10.3847/2041-8213/ab65c7⟩
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2020, 889 (1), pp.L1. ⟨10.3847/2041-8213/ab65c7⟩
The Astrophysical journal letters, 2020, 889 (1), pp.L1. ⟨10.3847/2041-8213/ab65c7⟩
Astrophys.J.
Astrophys.J., 2020, 889 (1), pp.L1. ⟨10.3847/2041-8213/ab65c7⟩
The Astrophysical Journal
The Astrophysical Journal Letters, 889(1), L1
Astrophysical journal, 2020, Vol.889(1), pp.L1 [Peer Reviewed Journal]
Supermassive black holes (SMBHs) are thought to provide energy that prevents catastrophic cooling in the centers of massive galaxies and galaxy clusters. However, it remains unclear how this "feedback" process operates. We use high-resolution optical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a577d596f5d4a8c8f961e8e3fa388b03
https://hal.archives-ouvertes.fr/hal-02416919
https://hal.archives-ouvertes.fr/hal-02416919
Autor:
Alastair C. Edge, M. T. Hogan, G. B. Taylor, Jeremy S. Sanders, M. Prasow-Émond, Andrew C. Fabian, Rodrigo Nemmen, M. Latulippe, Marie-Lou Gendron-Marsolais, Carter Rhea, Julie Hlavacek-Larrondo, A. Richard-Laferrière, G. Demontigny
A variety of large-scale diffuse radio structures have been identified in many clusters with the advent of new state-of-the-art facilities in radio astronomy. Among these diffuse radio structures, radio mini-halos are found in the central regions of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6b87413edb14951d293bf3909d8aa261