Multi-Conjugate Adaptive Optics VLT imaging of the distant old open cluster FSR 1415
Contribuinte(s) |
UNIVERSIDADE DE SÃO PAULO |
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Data(s) |
19/10/2012
19/10/2012
2008
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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 |
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 |