[HTML][HTML] Baryon cycles in the biggest galaxies
The universe's biggest galaxies have both vast atmospheres and supermassive central
black holes. This article reviews how those two components of a large galaxy couple and …
black holes. This article reviews how those two components of a large galaxy couple and …
Observational evidence of active galactic nuclei feedback
AC Fabian - Annual Review of Astronomy and Astrophysics, 2012 - annualreviews.org
Radiation, winds, and jets from the active nucleus of a massive galaxy can interact with its
interstellar medium, and this can lead to ejection or heating of the gas. This terminates star …
interstellar medium, and this can lead to ejection or heating of the gas. This terminates star …
First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback
D Nelson, A Pillepich, V Springel… - Monthly Notices of …, 2019 - academic.oup.com
We present the new TNG50 cosmological, magnetohydrodynamical simulation–the third and
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …
On the quenching of star formation in observed and simulated central galaxies: evidence for the role of integrated AGN feedback
In this paper, we investigate how massive central galaxies cease their star formation by
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …
The quiescent intracluster medium in the core of the Perseus cluster
Nature, 2016 - nature.com
Clusters of galaxies are the most massive gravitationally bound objects in the Universe and
are still forming. They are thus important probes of cosmological parameters and many …
are still forming. They are thus important probes of cosmological parameters and many …
How do central and satellite galaxies quench?–Insights from spatially resolved spectroscopy in the MaNGA survey
We investigate how star formation quenching proceeds within central and satellite galaxies
using spatially resolved spectroscopy from the SDSS-IV MaNGA DR15. We adopt a …
using spatially resolved spectroscopy from the SDSS-IV MaNGA DR15. We adopt a …
On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties
PN Best, TM Heckman - Monthly Notices of the Royal …, 2012 - academic.oup.com
A sample of 18 286 radio-loud active galactic nuclei (AGN) is presented, constructed by
combining the seventh data release of the Sloan Digital Sky Survey with the NRAO (National …
combining the seventh data release of the Sloan Digital Sky Survey with the NRAO (National …
Mechanical feedback from active galactic nuclei in galaxies, groups and clusters
BR McNamara, PEJ Nulsen - New Journal of Physics, 2012 - iopscience.iop.org
The radiative cooling timescales at the centers of hot atmospheres surrounding elliptical
galaxies, groups and clusters are much shorter than their ages. Therefore, hot atmospheres …
galaxies, groups and clusters are much shorter than their ages. Therefore, hot atmospheres …
The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
We simulate the growth of galaxies and their central supermassive black holes by
implementing a suite of semi-analytic models on the output of the Millennium Run, a very …
implementing a suite of semi-analytic models on the output of the Millennium Run, a very …
Concept of the X-ray astronomy recovery mission
M Tashiro, H Maejima, K Toda, R Kelley… - … 2018: ultraviolet to …, 2018 - spiedigitallibrary.org
The ASTRO-H mission was designed and developed through an international collaboration
of JAXA, NASA, ESA, and the CSA. It was successfully launched on February 17, 2016, and …
of JAXA, NASA, ESA, and the CSA. It was successfully launched on February 17, 2016, and …