cluster of galaxies【天】 - PMC

Kareem El-Badry, Jeremy Bradford, Eliot Quataert, Marla Geha, Michael Boylan-Kolchin, Daniel R. Weisz, Andrew Wetzel, Philip F. Hopkins, T. K. Chan, Alex Fitts, Dušan Kereš, Claude-André Faucher-Giguére

Mon Not R Astron Soc. Author manuscript; available in PMC 2019 Jun 1.

Published in final edited form as: Mon Not R Astron Soc. 2018 Jun; 477(2): 1536–1548. Published online 2018 Mar 24. doi: 10.1093/mnras/sty730

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A trail of dark-matter-free galaxies from a bullet-dwarf collision

Pieter van Dokkum, Zili Shen, Michael A. Keim, Sebastian Trujillo-Gomez, Shany Danieli, Dhruba Dutta Chowdhury, Roberto Abraham, Charlie Conroy, J. M. Diederik Kruijssen, Daisuke Nagai, Aaron Romanowsky

Nature. 2022; 605(7910): 435–439. Published online 2022 May 18. doi: 10.1038/s41586-022-04665-6

PMCID:: PMC9117144

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The origin of ultra diffuse galaxies: stellar feedback and quenching

T. K. Chan, D. Kereš, A. Wetzel, P. F. Hopkins, C.-A. Faucher-Giguère, K. El-Badry, S. Garrison-Kimmel, M. Boylan-Kolchin

Mon Not R Astron Soc. Author manuscript; available in PMC 2019 Jul 1.

Published in final edited form as: Mon Not R Astron Soc. 2018 Jul; 478(1): 906–925. Published online 2018 May 4. doi: 10.1093/mnras/sty1153

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The Molecular Cloud Lifecycle

Mélanie Chevance, J. M. Diederik Kruijssen, Enrique Vazquez-Semadeni, Fumitaka Nakamura, Ralf Klessen, Javier Ballesteros-Paredes, Shu-ichiro Inutsuka, Angela Adamo, Patrick Hennebelle

Space Sci Rev. 2020; 216(4): 50. Published online 2020 Apr 28. doi: 10.1007/s11214-020-00674-x

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The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations

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Mon Not R Astron Soc. Author manuscript; available in PMC 2019 Dec 11.

Published in final edited form as: Mon Not R Astron Soc. 2018 Dec 11; 481(3): 4133–4157. Published online 2018 Sep 14. doi: 10.1093/mnras/sty2513

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Living Rev Relativ. 2018; 21(1): 2. Published online 2018 Apr 12. doi: 10.1007/s41114-017-0010-3

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Ian Robson, Wayne S. Holland, Per Friberg

R Soc Open Sci. 2017 Sep; 4(9): 170754. Published online 2017 Sep 6. doi: 10.1098/rsos.170754

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Overview of the LAMOST survey in the first decade

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Electromagnetic counterparts to massive black-hole mergers

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Living Rev Relativ. 2022; 25(1): 3. Published online 2022 Jun 24. doi: 10.1007/s41114-022-00037-8

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Detecting galaxy–filament alignments in the Sloan Digital Sky Survey III

Yen-Chi Chen, Shirley Ho, Jonathan Blazek, Siyu He, Rachel Mandelbaum, Peter Melchior, Sukhdeep Singh

Mon Not R Astron Soc. 2019 May; 485(2): 2492–2504. Published online 2019 Feb 26. doi: 10.1093/mnras/stz539

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Subaru Telescope —History, active/adaptive optics, instruments, and scientific achievements—

Masanori IYE

Proc Jpn Acad Ser B Phys Biol Sci. 2021 Jul 31; 97(7): 337–370. doi: 10.2183/pjab.97.019

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Carbonaceous dust grains seen in the first billion years of cosmic time

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Design For The First Narrowband Filter For The Dark Energy Camera: Optimizing The LAGER Survey For Z ~ 7 Galaxies

Zhen-Ya Zheng, James E. Rhoads, Junxian Wang, Sangeeta Malhotra, Alistair Walker, Thomas Mooney, Chunyan Jiang, Weida Hu, Pascale Hibon, Linhua Jiang, Leopoldo Infante, L. Felipe Barrientos, Gaspar Galaz, Francisco Valdes, William Wester, Huan Yang, Alicia Coughlin, Santosh Harish, Wenyong Kang, Ali Ahmad Khostovan, Xu Kong, Lucia A. Perez, John Pharo, Isak Wold, XianZhong Zheng

Publ Astron Soc Pac. Author manuscript; available in PMC 2021 Jan 26.

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Globular cluster formation and evolution in the context of cosmological galaxy assembly: open questions

Duncan A. Forbes, Nate Bastian, Mark Gieles, Robert A. Crain, J. M. Diederik Kruijssen, Søren S. Larsen, Sylvia Ploeckinger, Oscar Agertz, Michele Trenti, Annette M. N. Ferguson, Joel Pfeffer, Oleg Y. Gnedin

Proc Math Phys Eng Sci. 2018 Feb; 474(2210): 20170616. Published online 2018 Feb 14. doi: 10.1098/rspa.2017.0616

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Gas loss in simulated galaxies as they fall into clusters

Renyue Cen, Ana Roxana Pop, Neta A. Bahcall

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ETHOS – an effective theory of structure formation: predictions for the high-redshift Universe – abundance of galaxies and reionization

Mark R. Lovell, Jesús Zavala, Mark Vogelsberger, Xuejian Shen, Francis-Yan Cyr-Racine, Christoph Pfrommer, Kris Sigurdson, Michael Boylan-Kolchin, Annalisa Pillepich

Mon Not R Astron Soc. Author manuscript; available in PMC 2019 Jul 1.

Published in final edited form as: Mon Not R Astron Soc. 2018 Jul 1; 477(3): 2886–2899. Published online 2018 Mar 28. doi: 10.1093/mnras/sty818

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The distribution and lifetime of powerful radio galaxies as a function of environment and redshift

David Garofalo, Chandra B. Singh, Alexa Zack

Sci Rep. 2018; 8: 15097. Published online 2018 Oct 10. doi: 10.1038/s41598-018-33532-6

Correction in:: Sci Rep. 2019; 9: 6345.

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A Massive Dead Disk Galaxy in the Young Universe

Sune Toft, Johannes Zabl, Johan Richard, Anna Gallazzi, Stefano Zibetti, Moire Prescott, Claudio Grillo, Allison W.S. Man, Nicholas Y. Lee, Carlos Gómez-Guijarro, Mikkel Stockmann, Georgios Magdis, Charles L. Steinhardt

Nature. Author manuscript; available in PMC 2019 Apr 26.

Published in final edited form as: Nature. 2017 Jun 21; 546(7659): 510–513. doi: 10.1038/nature22388

PMCID:: PMC6485677

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PMC Images search for cluster of galaxies【天】

Fig. 2Six filaments of galaxies connected to the Virgo Cluster, F1 to F6.

The color dots show the galaxies that belong to the filaments, and the color lines draw the spines of the filaments. The color codes the distance from us to the galaxies and the spines (h is the Hubble parameter). The TA events above 5.7 × 10¹⁹ eV (large black dots), nearby galaxies within 50 Mpc (gray dots), the Virgo Cluster galaxies (dark gray dots), and the center of the TA hotspot (red square) are also shown.

Filaments of galaxies as a clue to the origin of ultrahigh-energy cosmic rays

Sci Adv. 2019 Jan;5(1):eaau8227.
Fig. 3.

Histograms of gas-rich galaxies as a function of the ratio of the radial velocity to the virial velocity for four radial ranges at z = 0–0.4: (0–0.25)r_vir (Lower Right), (0.25–0.5)r_vir (Lower Left), (0.5–1) r_vir (Upper Right), and (1–1.5)r_vir (Upper Left), where r_vir = r₂₀₀ is the virial radius of the cluster. Infalling galaxies have negative radial velocities, whereas outgoing galaxies have positive radial velocities. For each radial range, two thresholds for the gas-to-total baryon ratio are shown, g/b > 0.01 (green histograms) and g/b > 0.1 (red histograms), as well as all galaxies (purple histograms). The satellite galaxies in the sample have stellar masses >10¹⁰ M_⊙ and the clusters all have total masses >10¹³ M_⊙.

Gas loss in simulated galaxies as they fall into clusters

Proc Natl Acad Sci U S A. 2014 Jun 3;111(22):7914-7919.
Figure 2Comparison between the distribution of hot gas and galaxies in the region surrounding Abell 2744.

XMM-Newton image of Abell 2744 (same as ) with the position of member galaxies with spectroscopic redshift within ±5,000 km s^-1 from the cluster mean[]. The red dots show galaxies identified as cluster members and the red curves show galaxy number density contours.

The baryon content of the Cosmic Web

Nature. ;528(7580):105-107.
Fig. 1Hammer projection of nearby galaxies within 50 Mpc (gray dots) and TA UHECR events above 5.7 × 1019 eV (large black dots) in equatorial coordinates.

The concentration of galaxies, represented by dark gray dots, is the Virgo Cluster. The red square marks the center of the TA hotspot. The pink and sky blue lines indicate the Galactic and Supergalactic planes, respectively. The purple line indicates the field of view limit of the TA experiment.

Filaments of galaxies as a clue to the origin of ultrahigh-energy cosmic rays

Sci Adv. 2019 Jan;5(1):eaau8227.