Dynamical black hole masses of BL Lac objects from the Sloan Digital Sky Survey

We measure black hole masses for 71 BL Lac objects from the Sloan Digital Sky Survey with redshifts out to z~ 0.4. We perform spectral decompositions of their nuclei from their host galaxies and measure their stellar velocity dispersions. Black hole masses are then derived from the black hole mass -...

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Main Authors: Plotkin, Richard, Markoff, S., Trager, S., Anderson, S.
Format: Journal Article
Published: Oxford University Press 2011
Online Access:http://hdl.handle.net/20.500.11937/52454
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author Plotkin, Richard
Markoff, S.
Trager, S.
Anderson, S.
author_facet Plotkin, Richard
Markoff, S.
Trager, S.
Anderson, S.
author_sort Plotkin, Richard
building Curtin Institutional Repository
collection Online Access
description We measure black hole masses for 71 BL Lac objects from the Sloan Digital Sky Survey with redshifts out to z~ 0.4. We perform spectral decompositions of their nuclei from their host galaxies and measure their stellar velocity dispersions. Black hole masses are then derived from the black hole mass - stellar velocity dispersion relation. We find BL Lac objects host black holes of similar masses, ~108.5M?, with a dispersion of ±0.4dex, similar to the uncertainties on each black hole measurement. Therefore, all BL Lac objects in our sample have the same indistinguishable black hole mass. These 71 BL Lac objects follow the black hole mass-bulge luminosity relation, and their narrow range of host galaxy luminosities confirm previous claims that BL Lac host galaxies can be treated as standard candles. We conclude that the observed diversity in the shapes of BL Lac object spectral energy distributions is not strongly driven by black hole mass or host galaxy properties. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS.
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spelling curtin-20.500.11937-524542017-09-13T15:48:31Z Dynamical black hole masses of BL Lac objects from the Sloan Digital Sky Survey Plotkin, Richard Markoff, S. Trager, S. Anderson, S. We measure black hole masses for 71 BL Lac objects from the Sloan Digital Sky Survey with redshifts out to z~ 0.4. We perform spectral decompositions of their nuclei from their host galaxies and measure their stellar velocity dispersions. Black hole masses are then derived from the black hole mass - stellar velocity dispersion relation. We find BL Lac objects host black holes of similar masses, ~108.5M?, with a dispersion of ±0.4dex, similar to the uncertainties on each black hole measurement. Therefore, all BL Lac objects in our sample have the same indistinguishable black hole mass. These 71 BL Lac objects follow the black hole mass-bulge luminosity relation, and their narrow range of host galaxy luminosities confirm previous claims that BL Lac host galaxies can be treated as standard candles. We conclude that the observed diversity in the shapes of BL Lac object spectral energy distributions is not strongly driven by black hole mass or host galaxy properties. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS. 2011 Journal Article http://hdl.handle.net/20.500.11937/52454 10.1111/j.1365-2966.2010.18172.x Oxford University Press fulltext
spellingShingle Plotkin, Richard
Markoff, S.
Trager, S.
Anderson, S.
Dynamical black hole masses of BL Lac objects from the Sloan Digital Sky Survey
title Dynamical black hole masses of BL Lac objects from the Sloan Digital Sky Survey
title_full Dynamical black hole masses of BL Lac objects from the Sloan Digital Sky Survey
title_fullStr Dynamical black hole masses of BL Lac objects from the Sloan Digital Sky Survey
title_full_unstemmed Dynamical black hole masses of BL Lac objects from the Sloan Digital Sky Survey
title_short Dynamical black hole masses of BL Lac objects from the Sloan Digital Sky Survey
title_sort dynamical black hole masses of bl lac objects from the sloan digital sky survey
url http://hdl.handle.net/20.500.11937/52454