<p>Classical model of slim accretion disks predicts saturated luminosity which only linearly proportional to the accreting black hole mass. We should the evidence for this luminosity from the Lijiang reverberation mapping campaigns of narrow line Seyfert 1 galaxies. This lends an opportunity of using super-Eddington accreting massive black holes as cosmic candles for expansion history of the Universe.</p
We estimated black hole masses for 9 Seyfert 1 and 13 Seyfert 2 galaxies in the Palomar and CfA brig...
In this Letter, we present evidence suggesting that the absence or presence of hidden broad-line reg...
Narrow-line Seyfert 1 galaxies (NLS1s) are generally considered peculiar objects among the broad cla...
Classical model of slim accretion disks predicts saturated luminosity which only linearly proportion...
International audienceWe use the BH masses deduced from the empirical relation of Kaspi et al. (2000...
We use the BH masses deduced from the empirical relation of Kaspi et al. (2000) between the size ...
We present a detailed model of an extreme slim disk (ESD) with a hot corona around a massive black ...
We discuss distinctive features of luminous accretion disks shining at the Eddington luminosity in t...
International audienceNarrow-Line Seyfert 1 galaxies (NLS1s) and Narrow-Line quasars (NLQs) seem to ...
In this Letter, we present evidence suggesting that the absence or presence of hidden broad-line reg...
We reexamine the locus of narrow-line Seyfert 1 galaxies (NLS1s) on theMBH- (black hole mass–bulge ...
We show that black holes grow substantially by accretion at close to Eddington rates. Using a comple...
International audienceIn a previous paper, Collin & Huré (\cite{Collin2001e}), using a sample of Act...
Reverberation mapping is the principal method for determining the masses of the central black holes ...
""\\"In the past few years, more and more pieces of evidence have been presented for a revision of t...
We estimated black hole masses for 9 Seyfert 1 and 13 Seyfert 2 galaxies in the Palomar and CfA brig...
In this Letter, we present evidence suggesting that the absence or presence of hidden broad-line reg...
Narrow-line Seyfert 1 galaxies (NLS1s) are generally considered peculiar objects among the broad cla...
Classical model of slim accretion disks predicts saturated luminosity which only linearly proportion...
International audienceWe use the BH masses deduced from the empirical relation of Kaspi et al. (2000...
We use the BH masses deduced from the empirical relation of Kaspi et al. (2000) between the size ...
We present a detailed model of an extreme slim disk (ESD) with a hot corona around a massive black ...
We discuss distinctive features of luminous accretion disks shining at the Eddington luminosity in t...
International audienceNarrow-Line Seyfert 1 galaxies (NLS1s) and Narrow-Line quasars (NLQs) seem to ...
In this Letter, we present evidence suggesting that the absence or presence of hidden broad-line reg...
We reexamine the locus of narrow-line Seyfert 1 galaxies (NLS1s) on theMBH- (black hole mass–bulge ...
We show that black holes grow substantially by accretion at close to Eddington rates. Using a comple...
International audienceIn a previous paper, Collin & Huré (\cite{Collin2001e}), using a sample of Act...
Reverberation mapping is the principal method for determining the masses of the central black holes ...
""\\"In the past few years, more and more pieces of evidence have been presented for a revision of t...
We estimated black hole masses for 9 Seyfert 1 and 13 Seyfert 2 galaxies in the Palomar and CfA brig...
In this Letter, we present evidence suggesting that the absence or presence of hidden broad-line reg...
Narrow-line Seyfert 1 galaxies (NLS1s) are generally considered peculiar objects among the broad cla...