Properties of the Line-of-sight Velocity Field in the Hot and X-Ray-emitting Circumgalactic Medium of Nearby Simulated Disk Galaxies

Autor: John A. ZuHone, Gerrit Schellenberger, Anna Ogorzałek, Benjamin D. Oppenheimer, Jonathan Stern, Ákos Bogdán, Nhut Truong, Maxim Markevitch, Annalisa Pillepich, Dylan Nelson, Joseph N. Burchett, Ildar Khabibullin, Caroline A. Kilbourne, Ralph P. Kraft, Paul E. J. Nulsen, Sylvain Veilleux, Mark Vogelsberger, Q. Daniel Wang, Irina Zhuravleva

Publikováno v: The Astrophysical Journal, Vol 967, Iss 1, p 49 (2024)

The hot, X-ray-emitting phase of the circumgalactic medium of massive galaxies is believed to be the reservoir of baryons from which gas flows onto the central galaxy and into which feedback from active galactic nuclei and stars inject mass, momentum

Externí odkaz: https://doaj.org/article/f4539e1a93ab4d52a110df75797b72fb

AMUSE-Antlia. I. Nuclear X-Ray Properties of Early-type Galaxies in a Dynamically Young Galaxy Cluster

Autor: Zhensong Hu, Yuanyuan Su, Zhiyuan Li, Kelley M. Hess, Ralph P. Kraft, William R. Forman, Paul E. J. Nulsen, Sarrvesh S. Sridhar, Andra Stroe, Junhyun Baek, Aeree Chung, Dirk Grupe, Hao Chen, Jimmy A. Irwin, Christine Jones, Scott W. Randall, Elke Roediger

Publikováno v: The Astrophysical Journal, Vol 956, Iss 2, p 104 (2023)

To understand the formation and growth of supermassive black holes (SMBHs) and their coevolution with host galaxies, it is essential to know the impact of environment on the activity of active galactic nuclei (AGNs). We present new Chandra X-ray obse

Externí odkaz: https://doaj.org/article/8264a484f05d4b689b6d5ac21856174f

The structure of cluster merger shocks: turbulent width and the electron heating timescale

Autor: H R Russell, P E J Nulsen, D Caprioli, U Chadayammuri, A C Fabian, M W Kunz, B R McNamara, J S Sanders, A Richard-Laferrière, M Beleznay, R E A Canning, J Hlavacek-Larrondo, L J King

We present a new 2 Ms Chandra observation of the cluster merger Abell 2146, which hosts two huge M~2 shock fronts each ~500 kpc across. For the first time, we resolve and measure the width of cluster merger shocks. The best-fit width for the bow shoc

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f2462ab4c4030f43973c531a961d430

Molecular gas along a bright H$\alpha$ filament in 2A 0335+096 revealed by ALMA

Autor: Robert Main, P. E. J. Nulsen, Jeremy S. Sanders, Francoise Combes, A. C. Edge, Christopher P. O'Dea, Stefi A. Baum, J. B. R. Oonk, A. C. Fabian, P. Salomé, I. J. Parrish, Brian R. McNamara, A. N. Vantyghem, Grant R. Tremblay, Norm Murray, Megan Donahue, M. T. Hogan, G. M. Voit, Robert W. O'Connell, Helen Russell

Publikováno v: Astrophysical journal, 2016, Vol.832(2), pp.148 [Peer Reviewed Journal]
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2016, 832 (2), pp.148. ⟨10.3847/0004-637X/832/2/148⟩
The Astrophysical Journal, 2016, 832 (2), pp.148. ⟨10.3847/0004-637X/832/2/148⟩

We present ALMA CO(1-0) and CO(3-2) observations of the brightest cluster galaxy (BCG) in the 2A 0335+096 galaxy cluster (z = 0.0346). The total molecular gas mass of (1.13+/-0.15) x 10^9 M_sun is divided into two components: a nuclear region and a 7

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d8b66d14421693e9b67f1ecca6ce4b38
https://www.repository.cam.ac.uk/handle/1810/262084

ACHANDRAOBSERVATION OF 3C 288—REHEATING THE COOL CORE OF A 3 keV CLUSTER FROM A NUCLEAR OUTBURST atz= 0.246

Autor: R. P. Kraft, Daniel A. Evans, Dharam V. Lal, P. E. J. Nulsen, Martin J. Hardcastle, Julia C. Lee, William R. Forman, Judith H. Croston, C. Jones

Publikováno v: The Astrophysical Journal. 722:1735-1743

We present results from a 42 ks Chandra/ACIS-S observation of the transitional FRI/FRII radio galaxy 3C288 at z = 0.246. We detect $\sim$3 keV gas extending to a radius of $\sim$0.5 Mpc with a 0.5-2.0 keV luminosity of 6.6 $\times$ 10$^{43}$ ergs s$^

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb4e9a1e38f2495d08d051d208def380
https://doi.org/10.1088/0004-637x/722/2/1735