Gemini/GMOS spectroscopy of the spheroid and globular cluster system of NGC 3923

We present a technique to extract ultra-deep diffuse-light spectra from the standard multi-object spectroscopic observations used to investigate extragalactic globular cluster (GC) systems. This technique allows a clean extraction of the spectrum of the host galaxy diffuse light from the same slitle...

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Autores principales: Norris, Mark A., Sharples, Ray M., Bridges, Terry, Gebhardt, Karl, Forbes, Duncan A., Proctor, Robert, Faifer, Favio Raúl, Forte, Juan Carlos, Beasley, Michael A., Zepf, Stephen E., Hanes, David A.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2008
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/84781
Aporte de:
id I19-R120-10915-84781
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Galaxies: abundances
Galaxies: general
Galaxies: individual: NGC 3923
Galaxies: stellar content
Globular clusters: general
spellingShingle Ciencias Astronómicas
Galaxies: abundances
Galaxies: general
Galaxies: individual: NGC 3923
Galaxies: stellar content
Globular clusters: general
Norris, Mark A.
Sharples, Ray M.
Bridges, Terry
Gebhardt, Karl
Forbes, Duncan A.
Proctor, Robert
Faifer, Favio Raúl
Forte, Juan Carlos
Beasley, Michael A.
Zepf, Stephen E.
Hanes, David A.
Gemini/GMOS spectroscopy of the spheroid and globular cluster system of NGC 3923
topic_facet Ciencias Astronómicas
Galaxies: abundances
Galaxies: general
Galaxies: individual: NGC 3923
Galaxies: stellar content
Globular clusters: general
description We present a technique to extract ultra-deep diffuse-light spectra from the standard multi-object spectroscopic observations used to investigate extragalactic globular cluster (GC) systems. This technique allows a clean extraction of the spectrum of the host galaxy diffuse light from the same slitlets as the GC targets. We show the utility of the method for investigating the kinematics and stellar populations of galaxies at radii much greater than usually probed in longslit studies, at no additional expense in terms of telescope time. To demonstrate this technique, we present Gemini South Multi-Object Spectrograph (GMOS) spectroscopy of 29 GCs associated with the elliptical galaxy NGC 3923. We compare the measured stellar population parameters of the GC system with those of the spheroid of NGC 3923 at the same projected radii, and find the GCs to have old ages >10 Gyr, [α/Fe] ∼ 0.3 and a range of metallicities running from [Z/H] = -1.8 to +0.35. The diffuse light of the galaxy is found to have ages, metallicities and [α/Fe] abundance ratios indistinguishable from those of the red GCs.
format Articulo
Articulo
author Norris, Mark A.
Sharples, Ray M.
Bridges, Terry
Gebhardt, Karl
Forbes, Duncan A.
Proctor, Robert
Faifer, Favio Raúl
Forte, Juan Carlos
Beasley, Michael A.
Zepf, Stephen E.
Hanes, David A.
author_facet Norris, Mark A.
Sharples, Ray M.
Bridges, Terry
Gebhardt, Karl
Forbes, Duncan A.
Proctor, Robert
Faifer, Favio Raúl
Forte, Juan Carlos
Beasley, Michael A.
Zepf, Stephen E.
Hanes, David A.
author_sort Norris, Mark A.
title Gemini/GMOS spectroscopy of the spheroid and globular cluster system of NGC 3923
title_short Gemini/GMOS spectroscopy of the spheroid and globular cluster system of NGC 3923
title_full Gemini/GMOS spectroscopy of the spheroid and globular cluster system of NGC 3923
title_fullStr Gemini/GMOS spectroscopy of the spheroid and globular cluster system of NGC 3923
title_full_unstemmed Gemini/GMOS spectroscopy of the spheroid and globular cluster system of NGC 3923
title_sort gemini/gmos spectroscopy of the spheroid and globular cluster system of ngc 3923
publishDate 2008
url http://sedici.unlp.edu.ar/handle/10915/84781
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