HST unveils a compact mildly relativistic broad-line region in the candidate true type 2 NGC 3147. (11th July 2019)

• Record Type: Journal Article
• Authors: Bianchi, Stefano; Antonucci, Robert; Capetti, Alessandro; Chiaberge, Marco; Laor, Ari; Bassani, Loredana; Carrera, Francisco J; La Franca, Fabio; Marinucci, Andrea; Matt, Giorgio; Middei, Riccardo; Panessa, Francesca
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 488:Number 1(2019)
• Page Start: L1
• Page End: L5
• Publication Date: 2019-07-11
• Subjects: galaxies: active -- galaxies: individual: NGC3147 -- galaxies: Seyfert; Astronomy -- Research -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnrasl/slz080
• Languages: English
• ISSNs: 1745-3933

Abstract

ABSTRACT: NGC 3147 has been considered the best case of a true type 2 AGN: an unobscured AGN, based on the unabsorbed compact X-ray continuum, which lacks a broad-line region (BLR). However, the very low luminosity of NGC 3147 implies a compact BLR, which produces very broad lines, hard to detect against the dominant background host galaxy. Narrow (0.1 arcsec × 0.1 arcsec) slit HST spectroscopy allowed us to exclude most of the host galaxy light, and revealed an H α line with an extremely broad base (FWZI${\sim }27\, 000$ km s −1 ). The line profile shows a steep cut-off blue wing and an extended red wing, which match the signature of a mildly relativistic thin accretion disc line profile. It is indeed well fit with a nearly face on thin disc, at i ∼ 23 °, with an inner radius at 77 ± 15 r g, which matches the prediction of $62^{+18}_{-14}$ r g from the R BLR – L 1/2 relation. This result questions the very existence of true type 2 AGN. Moreover, the detection of a thin disc, which extends below 100 r g in an L / L Edd ∼ 10 −4 system, contradicts the current view of the accretion flow configuration at extremely low accretion rates.