Dust and the intrinsic spectral index of quasar variations: hints of finite stress at the innermost stable circular orbit
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Dust and the intrinsic spectral index of quasar variations : hints of finite stress at the innermost stable circular orbit. / Weaver, John R.; Horne, Keith.
In: Monthly Notices of the Royal Astronomical Society, Vol. 512, No. 1, 17.03.2022, p. 899-916.Research output: Contribution to journal › Journal article › Research › peer-review
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TY - JOUR
T1 - Dust and the intrinsic spectral index of quasar variations
T2 - hints of finite stress at the innermost stable circular orbit
AU - Weaver, John R.
AU - Horne, Keith
PY - 2022/3/17
Y1 - 2022/3/17
N2 - We present a study of 9 242 spectroscopically confirmed quasars with multiepoch ugriz photometry from the SDSS Southern Survey. By fitting a separable linear model to each quasar's spectral variations, we decompose their five-band spectral energy distributions into variable (disc) and non-variable (host galaxy) components. In modelling the disc spectra, we include attenuation by dust on the line of sight through the host galaxy to its nucleus. We consider five commonly used attenuation laws, and find that the best description is by dust similar to that of the Small Magellanic Cloud, inferring a lack of carbonaceous grains from the relatively weak 2175-angstrom absorption feature. We go on to construct a composite spectrum for the quasar variations spanning 700-8000 angstrom. By varying the assumed power-law L-nu proportional to nu(alpha) spectral slope, we find a best-fitting value alpha = 0.71 +/- 0.02, excluding at high confidence the canonical L-nu proportional to nu(1/3) prediction for a steady-state accretion disc with a T proportional to r(-3/4) temperature profile. The bluer spectral index of the observed quasar variations instead supports the model of Agol & Krolik, and Mummery & Balbus, in which a steeper temperature profile, T proportional to r(-7/8), develops as a result of finite magnetically induced stress at the innermost stable circular orbit extracting energy and angular momentum from the black hole spin.
AB - We present a study of 9 242 spectroscopically confirmed quasars with multiepoch ugriz photometry from the SDSS Southern Survey. By fitting a separable linear model to each quasar's spectral variations, we decompose their five-band spectral energy distributions into variable (disc) and non-variable (host galaxy) components. In modelling the disc spectra, we include attenuation by dust on the line of sight through the host galaxy to its nucleus. We consider five commonly used attenuation laws, and find that the best description is by dust similar to that of the Small Magellanic Cloud, inferring a lack of carbonaceous grains from the relatively weak 2175-angstrom absorption feature. We go on to construct a composite spectrum for the quasar variations spanning 700-8000 angstrom. By varying the assumed power-law L-nu proportional to nu(alpha) spectral slope, we find a best-fitting value alpha = 0.71 +/- 0.02, excluding at high confidence the canonical L-nu proportional to nu(1/3) prediction for a steady-state accretion disc with a T proportional to r(-3/4) temperature profile. The bluer spectral index of the observed quasar variations instead supports the model of Agol & Krolik, and Mummery & Balbus, in which a steeper temperature profile, T proportional to r(-7/8), develops as a result of finite magnetically induced stress at the innermost stable circular orbit extracting energy and angular momentum from the black hole spin.
KW - accretion
KW - accretion discs
KW - methods: statistical
KW - ACTIVE GALACTIC NUCLEI
KW - DIGITAL SKY SURVEY
KW - LARGE-MAGELLANIC-CLOUD
KW - STAR-FORMING GALAXIES
KW - INTERSTELLAR EXTINCTION
KW - CONTINUUM EMISSION
KW - SPACE TELESCOPE
KW - BLACK-HOLE
KW - ULTRAVIOLET
KW - ACCRETION
U2 - 10.1093/mnras/stac248
DO - 10.1093/mnras/stac248
M3 - Journal article
VL - 512
SP - 899
EP - 916
JO - Royal Astronomical Society. Monthly Notices
JF - Royal Astronomical Society. Monthly Notices
SN - 0035-8711
IS - 1
ER -
ID: 302382145