Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-23T07:12:28.104Z Has data issue: false hasContentIssue false
  • English
  • Français

Globular clusters in the Fornax cluster: A report from the FDS survey

Published online by Cambridge University Press:  11 March 2020

Michele Cantiello Open the ORCID record for Michele Cantiello [Opens in a new window] ,
A. Venhola ,
M. Paolillo Open the ORCID record for M. Paolillo [Opens in a new window] ,
R. D’Abrusco ,
A. Grado ,
E. Iodice ,
R. Peletier ,
M. Capaccioli ,
M. Hilker Open the ORCID record for M. Hilker [Opens in a new window]  and
S. Mieske
...Show all authors
Michele Cantiello
Affiliation:
INAF Astronomical Observatory of Abruzzo, via Maggini snc, 64100Teramo, Italy email: [email protected]
A. Venhola
Affiliation:
University of Oulu, Finland
M. Paolillo
Affiliation:
University of Naples, Italy
R. D’Abrusco
Affiliation:
Center for Astrophysics, Harvard & Smithsonian, US
A. Grado
Affiliation:
INAF-Observatory of Naples, Italy
E. Iodice
Affiliation:
INAF-Observatory of Naples, Italy
R. Peletier
Affiliation:
Kapteyn Institute at the University of Groningen, Netherlands
M. Capaccioli
Affiliation:
University of Naples, Italy
M. Hilker
Affiliation:
ESO, Munich, Germany
S. Mieske
Affiliation:
ESO, Santiago, Chile
N. Napolitano
Affiliation:
Sun Yat-sen University, Guangzhou, P.R. China
G. Riccio
Affiliation:
University of Naples, Italy
M. Spavone
Affiliation:
INAF-Observatory of Naples, Italy
M. Quintini
Affiliation:
INAF Astronomical Observatory of Abruzzo, via Maggini snc, 64100Teramo, Italy email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Fornax Deep Survey (FDS) is a multi-band imaging survey of the Fornax cluster of galaxies, executed with the ESO VLT Survey Telescope (VST). The survey is designed to reach unprecedented surface brightness and point-source magnitude depth over one virial radius of the cluster. The scientific objectives of the survey are numerous: the study of the galaxy luminosity function, derivation of galaxy scaling relations, determination of the properties of compact stellar systems, an accurate determination of distances and 3-D geometry of the Fornax cluster, analysis of diffuse stellar light and galaxy interactions, etc.

In this contribute we give an overview on the interest of the survey on globular clusters (GC) populations, and present a report the status of the study of GCs also providing some preliminary results of our analysis, with particular regard to the two-dimensional distribution of GC candidates over ∼20 sq. degree area of Fornax centered on NGC 1399.

Keywords

Galaxies: star clustersgalaxies: clusters: individual (Fornax)galaxies: photometry
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S351: Star Clusters: From the Milky Way to the Early Universe , May 2019 , pp. 68 - 71
Copyright
© International Astronomical Union 2020

References

Ashman, K. M. & Zepf, S. E. 1998, Globular cluster systems (New York: Cambridge University Press)CrossRefGoogle Scholar
Bertin, E. & Arnouts, S. 1996, A&AS, 117, 393Google Scholar
Brodie, J. P. & Strader, J. 2006, ARA&A, 44, 193CrossRefGoogle Scholar
Cantiello, M., Brocato, E., & Blakeslee, J. P. 2009, A&A, 503, A87Google Scholar
Cantiello, M., D’Abrusco, R., Spavone, M., et al. 2018a, A&A, 611, A93Google Scholar
Cantiello, M., Grado, A., Rejkuba, M., et al. 2018b, A&A, 611, A21Google Scholar
D’Abrusco, R., Cantiello, M., Paolillo, M., et al. 2016, ApJL, 819, L31CrossRefGoogle Scholar
Drinkwater, M. J., Gregg, M. D. & Colless, M. 2001, ApJL, 548, L139CrossRefGoogle Scholar
Ferrarese, L., Côté, P., Cuillandre, J.-C., et al. 2012, ApJS, 200, 4CrossRefGoogle Scholar
Harris, W. E.Star Clusters: Saas-Fee Advanced Courses, Volume 28. ISBN 978-3-540-67646-1. Springer-Verlag Berlin Heidelberg, 2001, p. 223CrossRefGoogle Scholar
Iodice, E., Spavone, M., Capaccioli, M., et al. 2017a, ApJ, 839, 21CrossRefGoogle Scholar
Iodice, E., Spavone, M., Cantiello, M., et al. 2017b, ApJ, 851, 75CrossRefGoogle Scholar
Jordán, A., Peng, E. W., Blakeslee, J. P., et al. 2015, ApJS, 221, 13CrossRefGoogle Scholar
Misgeld, I. & Hilker, M. 2011, MNRAS, 414, 3699CrossRefGoogle Scholar
Mo, H., van den Bosch, F. C., & White, S. 2010, Galaxy Formation and Evolution (Cambridge, UK: Cambridge University Press)CrossRefGoogle Scholar
Pota, V., Napolitano, N. R., Hilker, M., et al. 2018, MNRAS, 481, 1744CrossRefGoogle Scholar
Riccio et al. 2019, https://arxiv.org/abs/1909.06383Google Scholar
Stetson, P. B. 1987, PASP, 99, 191CrossRefGoogle Scholar
Venhola, A., Peletier, R., Laurikainen, E., et al. 2018, A&A, 620, A165Google Scholar
West, M. J., Côté, P., Marzke, R. O., et al. 2004, Nature, 427, 31CrossRefGoogle Scholar