Next Article in Journal / Special Issue
Deep MOS Spectroscopy of NGC 1316 Globular Clusters
Previous Article in Journal / Special Issue
One Piece at a Time—Adding to the Puzzle of S0 Formation
Article Menu
Issue 3 (September) cover image

Export Article

Open AccessLetter

The Brazil–Argentina Gemini Group for the Study of Globular Cluster Systems (BAGGs GCs): FLAMINGOS-2 and GMOS Data for NGC 1395

Facultad de Ciencias Astronómicas y Geofísicas, National University of La Plata, La Plata B1900FWA, Argentina
Instituto de Astrofísica de La Plata (CCT La Plata, CONICET-UNLP), La Plata B1904CMC, Argentina
The National Scientific and Technical Research Council (CONICET), CABA C1425FQB, Argentina
Planetario de la Ciudad de Buenos Aires, CABA C1425FGC, Argentina
Departamento de Astronomia, Instituto de Física, Universidade Federal do Rio Grande do Sul, Porto Alegre 90040-060, Brazil
Instituto de Astronomia, Geofísica e Ciências Atmosféricas da U. de São Paulo, Cidade Universitária, 05508-900 São Paulo, Brazil
Author to whom correspondence should be addressed.
Current address: Paseo del Bosque s/n, La Plata CP B1900FWA, Argentina.
These authors contributed equally to this work.
Academic Editors: Duncan A. Forbes and Ericson D. Lopez
Galaxies 2017, 5(3), 38;
Received: 1 July 2017 / Revised: 3 August 2017 / Accepted: 7 August 2017 / Published: 14 August 2017
(This article belongs to the Special Issue On the Origin (and Evolution) of Baryonic Galaxy Halos)
PDF [435 KB, uploaded 15 August 2017]


In this letter, we present preliminary results of the analysis of Flamingos-2 and GMOS-S photometry of the globular cluster (GC) system of the elliptical galaxy NGC 1395. This is the first step of a long-term Brazilian–Argentinian collaboration for the study of GC systems in early-type galaxies. In the context of this collaboration, we obtained deep NIR photometric data in two different bands (J and K s), which were later combined with high quality optical Gemini + GMOS photometry previously obtained by the Argentinian team. This allowed us to obtain different color indices, less sensitive to the effect of horizontal branch (HB) stars for several hundreds of GC candidates, and to make an initial assessment of the presence or absence of multiple GC populations in colors in NGC 1395. View Full-Text
Keywords: early-type galaxies; globular cluster; galaxy halos early-type galaxies; globular cluster; galaxy halos

Figure 1

This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited (CC BY 4.0).
Printed Edition Available!
A printed edition of this Special Issue is available here.

Share & Cite This Article

MDPI and ACS Style

Faifer, F.; Escudero, C.; Smith Castelli, A.; Forte, J.; Sesto, L.; Chies Santos, A.; Cortesi, A.; Mendes de Oliveira, C. The Brazil–Argentina Gemini Group for the Study of Globular Cluster Systems (BAGGs GCs): FLAMINGOS-2 and GMOS Data for NGC 1395. Galaxies 2017, 5, 38.

Show more citation formats Show less citations formats

Note that from the first issue of 2016, MDPI journals use article numbers instead of page numbers. See further details here.

Related Articles

Article Metrics

Article Access Statistics



[Return to top]
Galaxies EISSN 2075-4434 Published by MDPI AG, Basel, Switzerland RSS E-Mail Table of Contents Alert
Back to Top