A Complex Stellar Line-of-Sight Velocity Distribution in the Lenticular Galaxy NGC 524

We present a detailed study of the stellar and gaseous kinematics in the luminous early-type galaxy NGC 524, derived from the long-slit spectroscopic observations obtained with the Russian 6 m telescope and the IFU data from the SAURON survey. The stellar line-of-sight velocity distribution (LOSVD)...

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Main Authors: Katkov I., Chilingarian I., Sil’chenko O., Zasov A., Afanasiev V.
Format: Article
Language:English
Published: De Gruyter 2011-09-01
Series:Open Astronomy
Subjects:
Online Access:https://doi.org/10.1515/astro-2017-0318
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author Katkov I.
Chilingarian I.
Sil’chenko O.
Zasov A.
Afanasiev V.
author_facet Katkov I.
Chilingarian I.
Sil’chenko O.
Zasov A.
Afanasiev V.
author_sort Katkov I.
collection DOAJ
description We present a detailed study of the stellar and gaseous kinematics in the luminous early-type galaxy NGC 524, derived from the long-slit spectroscopic observations obtained with the Russian 6 m telescope and the IFU data from the SAURON survey. The stellar line-of-sight velocity distribution (LOSVD) of NGC 524 exhibits strong asymmetry. We performed a comprehensive analysis of the LOSVD using two complementary approaches by the nbursts full spectral fitting technique: (a) a non-parametric LOSVD recovery and (b) a parametric recovery of two Gaussian kinematical components having different stellar populations. We discuss the origin of the complex stellar LOSVD of NGC 524.
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spelling doaj.art-e0b3f9ffb9324747b34e121c59f25ae72022-12-21T21:28:14ZengDe GruyterOpen Astronomy2543-63762011-09-0120345345810.1515/astro-2017-0318astro-2017-0318A Complex Stellar Line-of-Sight Velocity Distribution in the Lenticular Galaxy NGC 524Katkov I.0Chilingarian I.1Sil’chenko O.2Zasov A.3Afanasiev V.4Sternberg Astronomical Institute, Moscow State University, Universitetskii pr. 13, Moscow, 119992, Russian FederationCDS - Observatoire de Strasbourg, CNRS UMR 7550, Université de Strasbourg, 11 Rue de l'Université, 67000 Strasbourg, France Russian FederationSternberg Astronomical Institute, Moscow State University, Universitetskii pr. 13, Moscow, 119992, Rusian FederationSternberg Astronomical Institute, Moscow State University, Universitetskii pr. 13, Moscow, 119992, Rusian FederationSpecial Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, Karachaevo-Cherkesskaya Republic, 369167, Rusian FederationWe present a detailed study of the stellar and gaseous kinematics in the luminous early-type galaxy NGC 524, derived from the long-slit spectroscopic observations obtained with the Russian 6 m telescope and the IFU data from the SAURON survey. The stellar line-of-sight velocity distribution (LOSVD) of NGC 524 exhibits strong asymmetry. We performed a comprehensive analysis of the LOSVD using two complementary approaches by the nbursts full spectral fitting technique: (a) a non-parametric LOSVD recovery and (b) a parametric recovery of two Gaussian kinematical components having different stellar populations. We discuss the origin of the complex stellar LOSVD of NGC 524.https://doi.org/10.1515/astro-2017-0318galaxieskinematics and dynamicsindividual ngc 524
spellingShingle Katkov I.
Chilingarian I.
Sil’chenko O.
Zasov A.
Afanasiev V.
A Complex Stellar Line-of-Sight Velocity Distribution in the Lenticular Galaxy NGC 524
Open Astronomy
galaxies
kinematics and dynamics
individual ngc 524
title A Complex Stellar Line-of-Sight Velocity Distribution in the Lenticular Galaxy NGC 524
title_full A Complex Stellar Line-of-Sight Velocity Distribution in the Lenticular Galaxy NGC 524
title_fullStr A Complex Stellar Line-of-Sight Velocity Distribution in the Lenticular Galaxy NGC 524
title_full_unstemmed A Complex Stellar Line-of-Sight Velocity Distribution in the Lenticular Galaxy NGC 524
title_short A Complex Stellar Line-of-Sight Velocity Distribution in the Lenticular Galaxy NGC 524
title_sort complex stellar line of sight velocity distribution in the lenticular galaxy ngc 524
topic galaxies
kinematics and dynamics
individual ngc 524
url https://doi.org/10.1515/astro-2017-0318
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