Eight hundred new candidates for globular clusters in NGC5128 (Centaurus A)

Gretchen L H Harris, Matías Gómez, William E. Harris, Kyle Johnston, Farnoud Kazemzadeh, Wolfgang Kerzendorf, Doug Geisler, Kristin A. Woodley

Resultado de la investigación: Article

14 Citas (Scopus)

Resumen

We have used new wide-field imaging with the Magellan IMACS camera to search for globular cluster (GC) candidates around NGC5128, the nearest giant E galaxy. The imaging data are in the B and R broadband filters and cover a 1.55deg 2 field centered on the galaxy, corresponding to an area about 90 × 90 kpc 2 at the distance of NGC5128. All the fields were taken under exceptionally high-quality seeing conditions (FWHM = 04-05 in R). Using this material we are able, for the first time in the literature, to construct a homogeneous list of GC candidates covering a wide span of the NGC5128 halo and unusually free of field contaminants (foreground stars and faint background galaxies). Selecting the measured objects by color, magnitude, ellipticity, and profile size gives us a final catalog of 833 new high-quality GC candidates brighter than R = 21 (0.8 mag fainter than the standard GCluminosity function turnover point). The measured positions have better than 02 precision in both coordinates. This list can be used as the basis for spectroscopic follow-up, leading to a more comprehensive kinematic and dynamic study of the halo.

Idioma originalEnglish
Número de artículo84
PublicaciónAstronomical Journal
Volumen143
N.º4
DOI
EstadoPublished - abr 2012

Huella dactilar

globular clusters
turnover
kinematics
galaxies
filter
lists
pollutant
halos
ellipticity
catalogs
contaminants
coverings
cameras
broadband
color
filters
stars
profiles
material

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Citar esto

Harris, G. L. H., Gómez, M., Harris, W. E., Johnston, K., Kazemzadeh, F., Kerzendorf, W., ... Woodley, K. A. (2012). Eight hundred new candidates for globular clusters in NGC5128 (Centaurus A). Astronomical Journal, 143(4), [84]. https://doi.org/10.1088/0004-6256/143/4/84
Harris, Gretchen L H ; Gómez, Matías ; Harris, William E. ; Johnston, Kyle ; Kazemzadeh, Farnoud ; Kerzendorf, Wolfgang ; Geisler, Doug ; Woodley, Kristin A. / Eight hundred new candidates for globular clusters in NGC5128 (Centaurus A). En: Astronomical Journal. 2012 ; Vol. 143, N.º 4.
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Harris, GLH, Gómez, M, Harris, WE, Johnston, K, Kazemzadeh, F, Kerzendorf, W, Geisler, D & Woodley, KA 2012, 'Eight hundred new candidates for globular clusters in NGC5128 (Centaurus A)', Astronomical Journal, vol. 143, n.º 4, 84. https://doi.org/10.1088/0004-6256/143/4/84

Eight hundred new candidates for globular clusters in NGC5128 (Centaurus A). / Harris, Gretchen L H; Gómez, Matías; Harris, William E.; Johnston, Kyle; Kazemzadeh, Farnoud; Kerzendorf, Wolfgang; Geisler, Doug; Woodley, Kristin A.

En: Astronomical Journal, Vol. 143, N.º 4, 84, 04.2012.

Resultado de la investigación: Article

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N2 - We have used new wide-field imaging with the Magellan IMACS camera to search for globular cluster (GC) candidates around NGC5128, the nearest giant E galaxy. The imaging data are in the B and R broadband filters and cover a 1.55deg 2 field centered on the galaxy, corresponding to an area about 90 × 90 kpc 2 at the distance of NGC5128. All the fields were taken under exceptionally high-quality seeing conditions (FWHM = 04-05 in R). Using this material we are able, for the first time in the literature, to construct a homogeneous list of GC candidates covering a wide span of the NGC5128 halo and unusually free of field contaminants (foreground stars and faint background galaxies). Selecting the measured objects by color, magnitude, ellipticity, and profile size gives us a final catalog of 833 new high-quality GC candidates brighter than R = 21 (0.8 mag fainter than the standard GCluminosity function turnover point). The measured positions have better than 02 precision in both coordinates. This list can be used as the basis for spectroscopic follow-up, leading to a more comprehensive kinematic and dynamic study of the halo.

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