Are Narrow Line Seyfert 1 Galaxies powered by low mass black holes?. (arXiv:1907.02683v1 [astro-ph.GA])

Are Narrow Line Seyfert 1 Galaxies powered by low mass black holes?. (arXiv:1907.02683v1 [astro-ph.GA])
<a href="http://arxiv.org/find/astro-ph/1/au:+Viswanath_G/0/1/0/all/0/1">Gayathri Viswanath</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Stalin_C/0/1/0/all/0/1">C S Stalin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rakshit_S/0/1/0/all/0/1">Suvendu Rakshit</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kurian_K/0/1/0/all/0/1">Kshama S. Kurian</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Krishnan_U/0/1/0/all/0/1">Ujjwal Krishnan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gudennavar_S/0/1/0/all/0/1">Shivappa B. Gudennavar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kartha_S/0/1/0/all/0/1">Sreeja S. Kartha</a>

Narrow line Seyfert 1 galaxies (NLS1s) are believed to be powered by
accretion of matter onto low mass black holes (BHs) in spiral host galaxies
with BH masses M_BH of 10^6 – 10^8 M_sun . However, the broad band spectral
energy distribution of the gamma-ray emitting NLS1s are found to be similar to
flat spectrum radio quasars. This challenges our current notion of NLS1s having
low M_BH . To resolve this tension of low M_BH values in NLS1s, we fitted the
observed optical spectrum of a sample of radio-loud NLS1s (RL-NLS1s),
radio-quiet NLS1s (RQ-NLS1s) and radio-quiet broad line Seyfert 1 galaxies
(RQ-BLS1s) of about 500 each with the standard Shakura-Sunyaev accretion disk
(AD) model. For RL-NLS1s we found a mean log(M_ADBH/M_sun) of 7.98 +/- 0.54.
For RQ-NLS1s and RQ-BLS1s we found mean log(M_ADBH/M_sun) of 8.00 +/- 0.43 and
7.90 +/- 0.57, respectively. While the derived M_BH values of RQ-BLS1s are
similar to their virial masses, for NLS1s the derived M_ADBH values are about
an order of magnitude larger than their virial estimates. Our analysis thus
indicates that NLS1s have M_BH similar to RQ-BLS1s and their available virial
M_BH values are underestimated influenced by their observed relatively small
emission line widths. Considering Eddington ratio as an estimation of the
accretion rate and using M_ADBH, we found the mean accretion rate of our
RQ-NLS1s, RL-NLS1s and RQ-BLS1s as 0.06 (+0.16, -0.05), 0.05 (+0.18, -0.04) and
0.05 (+0.15, -0.04) respectively. Our results therefore suggest that NLS1s have
BH masses and accretion rates similar to BLS1s.

Narrow line Seyfert 1 galaxies (NLS1s) are believed to be powered by
accretion of matter onto low mass black holes (BHs) in spiral host galaxies
with BH masses M_BH of 10^6 – 10^8 M_sun . However, the broad band spectral
energy distribution of the gamma-ray emitting NLS1s are found to be similar to
flat spectrum radio quasars. This challenges our current notion of NLS1s having
low M_BH . To resolve this tension of low M_BH values in NLS1s, we fitted the
observed optical spectrum of a sample of radio-loud NLS1s (RL-NLS1s),
radio-quiet NLS1s (RQ-NLS1s) and radio-quiet broad line Seyfert 1 galaxies
(RQ-BLS1s) of about 500 each with the standard Shakura-Sunyaev accretion disk
(AD) model. For RL-NLS1s we found a mean log(M_ADBH/M_sun) of 7.98 +/- 0.54.
For RQ-NLS1s and RQ-BLS1s we found mean log(M_ADBH/M_sun) of 8.00 +/- 0.43 and
7.90 +/- 0.57, respectively. While the derived M_BH values of RQ-BLS1s are
similar to their virial masses, for NLS1s the derived M_ADBH values are about
an order of magnitude larger than their virial estimates. Our analysis thus
indicates that NLS1s have M_BH similar to RQ-BLS1s and their available virial
M_BH values are underestimated influenced by their observed relatively small
emission line widths. Considering Eddington ratio as an estimation of the
accretion rate and using M_ADBH, we found the mean accretion rate of our
RQ-NLS1s, RL-NLS1s and RQ-BLS1s as 0.06 (+0.16, -0.05), 0.05 (+0.18, -0.04) and
0.05 (+0.15, -0.04) respectively. Our results therefore suggest that NLS1s have
BH masses and accretion rates similar to BLS1s.

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