A FOSSIL BULGE GLOBULAR CLUSTER REVEALED BY VERY LARGE TELESCOPE MULTI-CONJUGATE ADAPTIVE OPTICS


Autoria(s): ORTOLANI, Sergio; BARBUY, Beatriz; MOMANY, Yazan; SAVIANE, Ivo; BICA, Eduardo; JILKOVA, Lucie; SALERNO, Gustavo M.; JUNGWIERT, Bruno
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

19/10/2012

19/10/2012

2011

Resumo

The globular cluster HP 1 is projected on the bulge, very close to the Galactic center. The Multi-Conjugate Adaptive Optics Demonstrator on the Very Large Telescope allowed us to acquire high-resolution deep images that, combined with first epoch New Technology Telescope data, enabled us to derive accurate proper motions. The cluster and bulge fields` stellar contents were disentangled through this process and produced an unprecedented definition in color-magnitude diagrams of this cluster. The metallicity of [Fe/H] approximate to -1.0 from previous spectroscopic analysis is confirmed, which together with an extended blue horizontal branch imply an age older than the halo average. Orbit reconstruction results suggest that HP 1 is spatially confined within the bulge.

CNPq

FAPESP

Identificador

ASTROPHYSICAL JOURNAL, v.737, n.1, 2011

0004-637X

http://producao.usp.br/handle/BDPI/27074

10.1088/0004-637X/737/1/31

http://dx.doi.org/10.1088/0004-637X/737/1/31

Idioma(s)

eng

Publicador

IOP PUBLISHING LTD

Relação

Astrophysical Journal

Direitos

restrictedAccess

Copyright IOP PUBLISHING LTD

Palavras-Chave #Galaxy: bulge #globular clusters: general #globular clusters: individual (HP 1) #COLOR-MAGNITUDE DIAGRAMS #HUBBLE-SPACE-TELESCOPE #GALACTIC BULGE #PROPER MOTION #SOLAR NEIGHBORHOOD #STELLAR ORBITS #BAADES WINDOW #STAR-CLUSTERS #BRANCH STARS #GIANT BRANCH #Astronomy & Astrophysics
Tipo

article

original article

publishedVersion