Hints on the Broad Line Region Structure of Quasars at High and Low Luminosities

Quasars show a considerable spectroscopic diversity. However, the variety of quasar spectra at low redshifts is non-random: a principal component analysis applied to large samples customarily identifies two main eigenvectors. In this contribution we show that the range of quasar optical spectral pro...

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Main Authors: Marziani Paola, Sulentic Jack W., Zamfir Sebastian, Negrete C. A., Dultzin Deborah
Format: Article
Language:English
Published: De Gruyter 2011-09-01
Series:Open Astronomy
Subjects:
Online Access:https://doi.org/10.1515/astro-2017-0322
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author Marziani Paola
Sulentic Jack W.
Zamfir Sebastian
Negrete C. A.
Dultzin Deborah
author_facet Marziani Paola
Sulentic Jack W.
Zamfir Sebastian
Negrete C. A.
Dultzin Deborah
author_sort Marziani Paola
collection DOAJ
description Quasars show a considerable spectroscopic diversity. However, the variety of quasar spectra at low redshifts is non-random: a principal component analysis applied to large samples customarily identifies two main eigenvectors. In this contribution we show that the range of quasar optical spectral properties observed at low-z and associated with the first eigenvector is preserved up to z ≈ 2 in a sample of high luminosity quasars. We also describe two major luminosity effects.
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spelling doaj.art-14f2cd5a9a8449e0b5b3d265686484a22022-12-21T22:40:31ZengDe GruyterOpen Astronomy2543-63762011-09-0120347247510.1515/astro-2017-0322astro-2017-0322Hints on the Broad Line Region Structure of Quasars at High and Low LuminositiesMarziani Paola0Sulentic Jack W.1Zamfir Sebastian2Negrete C. A.3Dultzin Deborah4INAF, Osservatorio Astronomico di Padova, Vicolo Osservatorio 5, Padova, I-35122, ItalyIAA-CSIC, Glorieta de Astronomia, 18008 Granada, SpainDept. of Physics & Astronomy, University of Wisconsin, 1848 Maria Dr., Stevens Point, WI 54481-1957, United States of AmericaInstituto de Astronomía UNAM, Ciudad Universitaria, Apt. Postal 70-264, México, DF, MexicoInstituto de Astronomía UNAM, Ciudad Universitaria, Apt. Postal 70-264, México, DF, MexicoQuasars show a considerable spectroscopic diversity. However, the variety of quasar spectra at low redshifts is non-random: a principal component analysis applied to large samples customarily identifies two main eigenvectors. In this contribution we show that the range of quasar optical spectral properties observed at low-z and associated with the first eigenvector is preserved up to z ≈ 2 in a sample of high luminosity quasars. We also describe two major luminosity effects.https://doi.org/10.1515/astro-2017-0322quasarsgeneral quasarsemission lines
spellingShingle Marziani Paola
Sulentic Jack W.
Zamfir Sebastian
Negrete C. A.
Dultzin Deborah
Hints on the Broad Line Region Structure of Quasars at High and Low Luminosities
Open Astronomy
quasars
general quasars
emission lines
title Hints on the Broad Line Region Structure of Quasars at High and Low Luminosities
title_full Hints on the Broad Line Region Structure of Quasars at High and Low Luminosities
title_fullStr Hints on the Broad Line Region Structure of Quasars at High and Low Luminosities
title_full_unstemmed Hints on the Broad Line Region Structure of Quasars at High and Low Luminosities
title_short Hints on the Broad Line Region Structure of Quasars at High and Low Luminosities
title_sort hints on the broad line region structure of quasars at high and low luminosities
topic quasars
general quasars
emission lines
url https://doi.org/10.1515/astro-2017-0322
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AT zamfirsebastian hintsonthebroadlineregionstructureofquasarsathighandlowluminosities
AT negreteca hintsonthebroadlineregionstructureofquasarsathighandlowluminosities
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