Multi-Conjugate Adaptive Optics VLT imaging of the distant old open cluster FSR 1415


Autoria(s): MOMANY, Y.; ORTOLANI, S.; BONATTO, C.; BICA, E.; BARBUY, B.
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

19/10/2012

19/10/2012

2008

Resumo

We employ the recently installed near-infrared Multi-Conjugate Adaptive Optics demonstrator (MAD) to determine the basic properties of a newly identified, old and distant, Galactic open cluster (FSR 1415). The MAD facility remarkably approaches the diffraction limit, reaching a resolution of 0.07 arcsec (in K), that is also uniform in a field of similar to 1.8 arcmin in diameter. The MAD facility provides photometry that is 50 per cent complete at K similar to 19. This corresponds to about 2.5 mag below the cluster main-sequence turn-off. This high-quality data set allows us to derive an accurate heliocentric distance of 8.6 kpc, a metallicity close to solar and an age of similar to 2.5 Gyr. On the other hand, the deepness of the data allows us to reconstruct (completeness-corrected) mass functions (MFs) indicating a relatively massive cluster, with a flat core MF. The Very Large Telescope/MAD capabilities will therefore provide fundamental data for identifying/analysing other faint and distant open clusters in the Galaxy III and IV quadrants.

CNPq

FAPESP

Italian Ministero dell`Universita e della Ricerca Scientifica e Tecnologica

Identificador

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v.391, n.4, p.1650-1658, 2008

0035-8711

http://producao.usp.br/handle/BDPI/27137

10.1111/j.1365-2966.2008.14019.x

http://dx.doi.org/10.1111/j.1365-2966.2008.14019.x

Idioma(s)

eng

Publicador

WILEY-BLACKWELL PUBLISHING, INC

Relação

Monthly Notices of the Royal Astronomical Society

Direitos

restrictedAccess

Copyright WILEY-BLACKWELL PUBLISHING, INC

Palavras-Chave #instrumentation: adaptive optics #techniques: photometric #stars: Population II #open clusters and associations: individual: FSR 1415 #infrared: stars #DWARF IRREGULAR GALAXY #MILKY-WAY DISK #STAR-CLUSTERS #GALACTIC-CENTER #STRUCTURAL PARAMETERS #STELLAR POPULATIONS #GLOBULAR-CLUSTERS #DYNAMICAL MODELS #INNER GALAXY #OVER-DENSITY #Astronomy & Astrophysics
Tipo

article

original article

publishedVersion