The total mass of the early-type galaxy NGC 4649 (M60)

In this paper the problem of the total mass and the total mass-to-light ratio of the early-type galaxy NGC 4649 (M60) is analyzed. Use is made of two independent techniques: the X-ray methodology which is based on the temperature of the X-ray halo of NGC 4649 and the tracer mass estimator (TME) whic...

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Main Authors: Samurović S., Ćirković M.M.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2008-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2008/1450-698X0877001S.pdf
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author Samurović S.
Ćirković M.M.
author_facet Samurović S.
Ćirković M.M.
author_sort Samurović S.
collection DOAJ
description In this paper the problem of the total mass and the total mass-to-light ratio of the early-type galaxy NGC 4649 (M60) is analyzed. Use is made of two independent techniques: the X-ray methodology which is based on the temperature of the X-ray halo of NGC 4649 and the tracer mass estimator (TME) which uses globular clusters (GCs) observed in this galaxy. The mass is calculated in Newtonian and Modified Newtonian Dynamics (MOND) approaches and it is found that inside 3 effective radii (Re ) there is no need for large amounts of dark matter. Beyond 3Re the dark matter starts to play important dynamical role. The possible reasons for the discrepancy between the estimates of the total mass based on X-rays and TME in the outer regions of NGC 4649 are also discussed.
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spelling doaj.art-50695aba1984408e8da27a5951e809842022-12-22T03:01:01ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X1820-92892008-01-0120081771710.2298/SAJ0877001S1450-698X0877001SThe total mass of the early-type galaxy NGC 4649 (M60)Samurović S.0Ćirković M.M.1Astronomical Observatory, BelgradeAstronomical Observatory, BelgradeIn this paper the problem of the total mass and the total mass-to-light ratio of the early-type galaxy NGC 4649 (M60) is analyzed. Use is made of two independent techniques: the X-ray methodology which is based on the temperature of the X-ray halo of NGC 4649 and the tracer mass estimator (TME) which uses globular clusters (GCs) observed in this galaxy. The mass is calculated in Newtonian and Modified Newtonian Dynamics (MOND) approaches and it is found that inside 3 effective radii (Re ) there is no need for large amounts of dark matter. Beyond 3Re the dark matter starts to play important dynamical role. The possible reasons for the discrepancy between the estimates of the total mass based on X-rays and TME in the outer regions of NGC 4649 are also discussed.http://www.doiserbia.nb.rs/img/doi/1450-698X/2008/1450-698X0877001S.pdfgravitationgalaxies: elliptical and lenticularCDgalaxies: kinematics and dynamicsgalaxies: individual: NGC 4649cosmology: dark matter
spellingShingle Samurović S.
Ćirković M.M.
The total mass of the early-type galaxy NGC 4649 (M60)
Serbian Astronomical Journal
gravitation
galaxies: elliptical and lenticular
CD
galaxies: kinematics and dynamics
galaxies: individual: NGC 4649
cosmology: dark matter
title The total mass of the early-type galaxy NGC 4649 (M60)
title_full The total mass of the early-type galaxy NGC 4649 (M60)
title_fullStr The total mass of the early-type galaxy NGC 4649 (M60)
title_full_unstemmed The total mass of the early-type galaxy NGC 4649 (M60)
title_short The total mass of the early-type galaxy NGC 4649 (M60)
title_sort total mass of the early type galaxy ngc 4649 m60
topic gravitation
galaxies: elliptical and lenticular
CD
galaxies: kinematics and dynamics
galaxies: individual: NGC 4649
cosmology: dark matter
url http://www.doiserbia.nb.rs/img/doi/1450-698X/2008/1450-698X0877001S.pdf
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