Pregled bibliografske jedinice broj: 614172
Radio Galaxy Feedback in X-ray-selected Groups from COSMOS: The Effect on the Intracluster Medium
Radio Galaxy Feedback in X-ray-selected Groups from COSMOS: The Effect on the Intracluster Medium // The Astrophysical journal, 714 (2010), 1; 218-228 doi:10.1088/0004-637X/714/1/218 (međunarodna recenzija, članak, znanstveni)
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Naslov
Radio Galaxy Feedback in X-ray-selected Groups from COSMOS: The Effect on the Intracluster Medium
Autori
Giodini, S. ; Smolčić, Vernesa ; Finoguenov, A. ; Boehringer, H. ; Bîrzan, L. ; Zamorani, G. ; Oklopčić, A. ; Pierini, D. ; Pratt, G.W. ; Schinnerer, E. ; Massey, R. ; Koekemoer, A. M. ; Salvato, M. ; Sanders, D. B. ; Kartaltepe, J. S. ; Thompson, D.
Izvornik
The Astrophysical journal (0004-637X) 714
(2010), 1;
218-228
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
intergalactic medium; galaxies: active; galaxies: clusters: general; radio continuum: galaxies; X-rays: galaxies: clusters
Sažetak
We quantify the importance of the mechanical energy released by radio galaxies inside galaxy groups. We use scaling relations to estimate the mechanical energy released by 16 radio-active galactic nuclei located inside X-ray-detected galaxy groups in the COSMOS field. By comparing this energy output to the host groups' gravitational binding energy, we find that radio galaxies produce sufficient energy to unbind a significant fraction of the intragroup medium. This unbinding effect is negligible in massive galaxy clusters with deeper potential wells. Our results correctly reproduce the breaking of self-similarity observed in the scaling relation between entropy and temperature for galaxy groups.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Ustanove:
Prirodoslovno-matematički fakultet, Zagreb
Profili:
Vernesa Smolčić
(autor)
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus