HST unveils a compact mildly relativistic Broad Line Region in the candidate true type 2 NGC 3147. (arXiv:1905.09627v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Bianchi_S/0/1/0/all/0/1">Stefano Bianchi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Antonucci_R/0/1/0/all/0/1">Robert Antonucci</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Capetti_A/0/1/0/all/0/1">Alessandro Capetti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chiaberge_M/0/1/0/all/0/1">Marco Chiaberge</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Laor_A/0/1/0/all/0/1">Ari Laor</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bassani_L/0/1/0/all/0/1">Loredana Bassani</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Carrera_F/0/1/0/all/0/1">Francisco J. Carrera</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Franca_F/0/1/0/all/0/1">Fabio La Franca</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Marinucci_A/0/1/0/all/0/1">Andrea Marinucci</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Matt_G/0/1/0/all/0/1">Giorgio Matt</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Middei_R/0/1/0/all/0/1">Riccardo Middei</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Panessa_F/0/1/0/all/0/1">Francesca Panessa</a>
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″x0.1″) slit HST spectroscopy
allowed us to exclude most of the host galaxy light, and revealed an H$alpha$
line with an extremely broad base (FWZI$sim27,000$ km s$^{-1}$). The line
profile shows a steep cutoff blue wing and an extended red wing, which match
the signature of a mildly relativistic thin accretion disk line profile. It is
indeed well fit with a nearly face on thin disk, at $isim23^circ$, with an
inner radius at $77pm15$ r$_g$, which matches the prediction of
$62^{+18}_{-14}$ r$_g$ from the $R_{rm BLR} sim L^{1/2}$ relation. This
result questions the very existence of true type 2 AGN. Moreover, the detection
of a thin disk, which extends below 100 r$_g$ in an $L/L_{rm Edd}sim10^{-4}$
system, contradicts the current view of the accretion flow configuration at
extremely low accretion rates.
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″x0.1″) slit HST spectroscopy
allowed us to exclude most of the host galaxy light, and revealed an H$alpha$
line with an extremely broad base (FWZI$sim27,000$ km s$^{-1}$). The line
profile shows a steep cutoff blue wing and an extended red wing, which match
the signature of a mildly relativistic thin accretion disk line profile. It is
indeed well fit with a nearly face on thin disk, at $isim23^circ$, with an
inner radius at $77pm15$ r$_g$, which matches the prediction of
$62^{+18}_{-14}$ r$_g$ from the $R_{rm BLR} sim L^{1/2}$ relation. This
result questions the very existence of true type 2 AGN. Moreover, the detection
of a thin disk, which extends below 100 r$_g$ in an $L/L_{rm Edd}sim10^{-4}$
system, contradicts the current view of the accretion flow configuration at
extremely low accretion rates.
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