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  5. Large-scale environment of FR 0 radio galaxies
 

Large-scale environment of FR 0 radio galaxies

Journal
ASTRONOMY & ASTROPHYSICS  
Date Issued
2020
Author(s)
Capetti, A.  
•
Massaro, F.  
•
BALDI, RANIERI DIEGO  
DOI
10.1051/0004-6361/201935962
Abstract
We explore the properties of the large-scale environment of the sources in the Faranoff-Riley class 0 catalog (FR0CAT). This sample includes 104 compact radio sources that are associated with nearby (z < 0.05) early-type galaxies. Using various estimators, we find that FR 0s are located in regions with higher than the average number of galaxies. The average galaxies density around FR 0s is a factor two lower with respect to FR I radio galaxies. This latter difference is driven by the large fraction (63%) of FR 0s that are located in groups formed by fewer than 15 galaxies. FR Is rarely (17%) inhabit an environment like this. In addition to the lack of substantial extended radio emission that defines the FR 0 class, this is the first significant difference between the properties of these two populations of low-power radio galaxies. We interpret the differences in environment between FR 0s and FR Is as due to an evolutionary link between local galaxies density, black hole spin, jet power, and extended radio emission.
Volume
633
Start page
A161
Uri
http://hdl.handle.net/20.500.12386/36302
Url
https://www.aanda.org/articles/aa/full_html/2020/01/aa35962-19/aa35962-19.html
Issn Identifier
0004-6361
Ads BibCode
2020A&A...633A.161C
Rights
open.access
File(s)
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capetti20b.pdf

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Size

335.38 KB

Format

Adobe PDF

Checksum (MD5)

c3c283447cc878866d600594baf20b51

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