The balance between shocks and AGN photoionization in radio sources and its relation to the radio size

Free access article

Issue		A&A Volume 383, Number 1, February III 2002


Page(s)		46 - 55
Section		Extragalactic astronomy
DOI		http://dx.doi.org/10.1051/0004-6361:20011727

A&A 383, 46-55 (2002)
DOI: 10.1051/0004-6361:20011727

The balance between shocks and AGN photoionization in radio sources and its relation to the radio size

E. Moy^{1, 2} and B. Rocca-Volmerange^{1, 3}

¹ Institut d'Astrophysique de Paris, 98bis boulevard Arago, 75014 Paris, France
² Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, 85741 Garching, Germany
³ Institut d'Astrophysique Spatiale, Bât. 121, Université Paris XI, 91405 Orsay, France

(Received 27 April 2001 / Accepted 26 November 2001 )

Abstract
We have analyzed the ultraviolet and optical emission line ratios of a large sample of extragalactic radio sources (QSOs and radio galaxies), with the help of models combining AGN photoionization and shocks. The results strongly suggest that the two ionizing mechanisms frequently coexist. The model sequences obtained by varying the balance between shocks and AGN photoionization account for most emission line data in the 12 line ratio diagrams we have considered. In the frequently used diagrams involving [OIII] $\lambda$ 5007/H $\beta$ , [OI] $\lambda$ 6300/H $\alpha$ , [NII] $\lambda$ 6584/H $\alpha$ and [SII] $\lambda\lambda$ 6716, 6731 (Veilleux & Osterbrock 1987), the effect of varying the shock-photoionization balance mimics a variation of the ionization parameter ( U) in traditional photoionization sequences. In most of the remaining diagrams, such as [OI] $\lambda$ 6300/[OIII] $\lambda$ 5007 vs. [OIII] $\lambda$ 4363/[OIII] $\lambda$ 5007, [OIII] $\lambda$ 5007/H $\beta$ vs. [OIII] $\lambda$ 4363/[OIII] $\lambda$ 5007 and CIII] $\lambda$ 1909/[CII] $\lambda$ 2326 vs. CIV $\lambda$ 1549/[CII] $\lambda$ 2326, the data can only be accounted for if both photoionization and shocks contribute to the line fluxes. The coexistence of shocks and AGN photoionization also provides an explanation for the most extreme objects in the NV $\lambda$ 1240/HeII $\lambda$ 1640 vs. NV $\lambda$ 1240/CIV $\lambda$ 1549 diagram without requiring largely super-solar metallicities. In addition, we show that there is a relationship between the [OII] $\lambda$ 3727/[OIII] $\lambda$ 5007 ratio (i.e., the ionization level of the gas) and the radio size in radio galaxies. This strongly supports the hypothesis that the most compact ( $\le$ 2kpc) and the largest ( $\ge$ 150 kpc) sources are dominated by photoionization, while intermediate-sized radio galaxies are dominated by shocks. We briefly discuss the possible origin of the relation between the shock-ionization balance and the radio size.

Key words: line: formation -- galaxies: active -- galaxies: evolution -- galaxies: ISM -- quasars: emission lines

Offprint request: E. Moy, moy@mpe.mpg.de

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