activity
20162021
most citedMeasuring bulk flows of the intracluster medium in the Perseus and Coma galaxy clusters using XMM-Newton

61 citations · 144 across the 4 of their papers we have counts for

collaborators

16 papers

astro-ph.GA20219 cited

A Massive, Clumpy Molecular Gas Distribution and Displaced AGN in Zw 3146

A. N. Vantyghem, B. R. McNamara, C. P. O'Dea +8

We present a recent ALMA observation of the CO(1-0) line emission in the central galaxy of the Zw 3146 galaxy cluster (). We also present updated X-ray cavity measurement…

astro-ph.CO201961 cited

Measuring bulk flows of the intracluster medium in the Perseus and Coma galaxy clusters using XMM-Newton

J. S. Sanders, K. Dennerl, H. R. Russell +7

We demonstrate a novel technique for calibrating the energy scale of the XMM EPIC-pn detector, which allows us to measure bulk flows in the intracluster medium (ICM) of the Perseus…

astro-ph.GA2019

Constraining cold accretion onto supermassive black holes: molecular gas in the cores of eight brightest cluster galaxies revealed by joint CO and CN absorption

Tom Rose, A. C. Edge, F. Combes +18

To advance our understanding of the fuelling and feedback processes which power the Universe's most massive black holes, we require a significant increase in our knowledge of the m…

hep-ph2019

Astrophysical limits on very light axion-like particles from Chandra grating spectroscopy of NGC 1275

Christopher S. Reynolds, M. C. David Marsh, Helen R. Russell +4

Axions/axion-like particles (ALPs) are a well motivated extension of the Standard Model and are generic within String Theory. The X-ray transparency of the intracluster medium (ICM…

astro-ph.GA2019

Anatomy of a Cooling Flow: The Feedback Response to Pure Cooling in the Core of the Phoenix Cluster

M. McDonald, B. R. McNamara, G. M. Voit +17

We present new, deep observations of the Phoenix cluster from the Chandra X-ray Observatory, the Hubble Space Telescope, and the Karl Jansky Very Large Array. These data provide an…

astro-ph.GA2019

Ubiquitous cold and massive filaments in cool core clusters

V. Olivares, P. Salomé, F. Combes +20

Multi-phase filamentary structures around Brightest Cluster Galaxies are likely a key step of AGN-feedback. We observed molecular gas in 3 cool cluster cores: Centaurus, Abell S110…