Ionized outflows in luminous type 2 AGNs at z < 0.6: no evidence for significant impact on the host galaxies. Issue 1 (17th April 2016)

• Record Type: Journal Article
• Authors: Villar-Martín, M.; Arribas, S.; Emonts, B.; Humphrey, A.; Tadhunter, C.; Bessiere, P.; Cabrera Lavers, A.; Ramos Almeida, C.
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 460:Issue 1(2016)
• Page Start: 130
• Page End: 162
• Publication Date: 2016-04-17
• Subjects: galaxies: active -- galaxies: evolution -- quasars: emission lines -- quasars: general; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stw901
• Languages: English
• ISSNs: 0035-8711

Abstract

Abstract: We investigate the presence of extended ionized outflows in 18 luminous type 2 AGNs (11 quasars and 7 high-luminosity Seyfert 2s) at 0.3 &lt; z &lt; 0.6 based on VLT-FORS2 spectroscopy. We infer typical lower limits on the radial sizes of the outflows R o ≳ several × 100 pc and upper limits R o ≲ 1–2 kpc. Our results are inconsistent with related studies which suggest that large scale ( R o ∼ several-15 kpc) are ubiquitous in QSO2. We study the possible causes of discrepancy and propose that seeing smearing is the cause of the large inferred sizes. The implications in our understanding of the feedback phenomenon are important since the mass M o (through the density), mass injection $\skew3\dot{M}_{\rm o}$ and energy injection $\dot{E}_{\rm o}$ rates of the outflows become highly uncertain. One conclusion seems unavoidable: M o, $\skew3\dot{M}_{\rm o}$ and $\dot{E}_{\rm o}$ are modest or low compared with previous estimations. We obtain typically M o ≲ (0.4–22) × 10 6 M⊙ (median 1.1 × 10 6 M⊙ ) assuming n = 1000 cm −3 . These are ∼10 2 –10 4 times lower than values reported in the literature. Even under the most favourable assumptions, we obtain $\skew3\dot{M}_{\rm o}\lesssim$ 10 M⊙ yr −1 in general, 100–1000 times lower than claimed in related studies. Although the uncertainties are large, it is probable that these are lower than typical star-forming rates. In conclusion, no evidence is found supporting that typical outflows can affect the interstellar medium of the host galaxies across spatial scales ≳ 1–2 kpc.