Spitzer mid-IR spectroscopy of powerful 2Jy and 3CRR radio galaxies. I. Evidence against a strong starburst-AGN connection in radio-loud AGN

Дата и время публикации : 2011-11-18T20:55:01Z

Авторы публикации и институты :
D. Dicken
C. Tadhunter
D. Axon
R. Morganti
A. Robinson
M. B. N. Kouwenhoven
H. Spoon
P. Kharb
K. J. Inskip
J. Holt
C. Ramos Almeida
N. P. H. Nesvadba

Ссылка на журнал-издание: Ссылка на журнал-издание не найдена
Коментарии к cтатье: 33 pages, 14 Figures, Accepted for publication in ApJ
Первичная категория: astro-ph.CO

Все категории : astro-ph.CO

Краткий обзор статьи: We present deep Spitzer/IRS spectra for complete samples of 46 2Jy radio galaxies (0.05<z<0.7) and 19 3CRR FRII radio galaxies (z<0.1), and use the detection of polycyclic aromatic hydrocarbon (PAH) features to examine the incidence of contemporaneous star formation and radio-loud AGN activity. Our analysis reveals PAH features in only a minority (30%) of the objects with good IRS spectra. Using the wealth of complementary data available for the 2Jy and 3CRR samples we make detailed comparisons between a range of star formation diagnostics: optical continuum spectroscopy, mid- to far-IR (MFIR) color, far-IR excess and PAH detection. There is good agreement between the various diagnostic techniques: most candidates identified to have star formation activity on the basis of PAH detection are also identified using at least two of the other techniques. We find that only 35% of the combined 2Jy and 3CRR sample show evidence for recent star formation activity (RSFA) at optical and/or MFIR wavelengths. This result argues strongly against the idea of a close link between starburst and powerful radio-loud AGN activity, reinforcing the view that, although a large fraction of powerful radio galaxies may be triggered in galaxy interactions, only a minority are triggered at the peaks of star formation activity in major, gas-rich mergers. However, we find that compact radio sources (D < 15 kpc) show a significantly higher incidence of RSFA (>75%) than their more extended counterparts (=15 — 25%). We discuss this result in the context of a possible bias towards the selection of compact radio sources triggered in gas-rich environments.

Category: Physics