paper

Chandra Observation of M84, Radio Lobe Elliptical in Virgo cluster

arXiv:astro-ph/0010450 · doi:10.1086/318910

Abstract

We analyzed a deep Chandra observation of M84, a bright elliptical galaxy in the core of the Virgo cluster. We find that the spatial distribution of the soft X-ray emission is defined by the radio structure of the galaxy. In particular we find two low density regions associated with the radio lobes and surrounded by higher density X-ray filaments. In addition to a central AGN and a population of galactic sources, we find a diffuse hard source filling the central 10 kpc region. Since the morphology of the hard source appears round and is different from that seen in the radio or in soft X-rays, we propose that it is hot gas heated by the central AGN. Finally, we find that the central elemental abundance in the X-ray gas is comparable to that measured optically.

accepted to ApJ Letters, Oct 2000. 5 pages in emulateapj

References in corpus (2)

Cited by in corpus (102)