Navegação Ciências Exatas e da Terra por Assunto "Globular clusters: general"
Resultados 21-30 de 30
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New SX Phe variables in the globular cluster NGC 288
(2015) [Artigo de periódico]We report the discovery of two new variable stars in the metal-poor globular cluster NGC 288, found by means of time series CCD photometry. We classified the new variables as SX Phoenicis (SX Phe) due to their characteristic ... -
NGC 6558 : a blue horizontal branch moderately metal-poor globular cluster in the bulge
(2007) [Artigo de periódico]We present, for the first time, a detailed abundance analysis of five giant stars in the moderately metal-poor bulge globular cluster NGC 6558. Spectra have been obtained at the VLT with the multifiber spectrograph FLAMES ... -
Optical-near-IR analysis of globular clusters in the IKN dwarf spheroidal : a complex star formation history
(2015) [Artigo de periódico]Context. Age, metallicity, and spatial distribution of globular clusters (GCs) provide a powerful tool for reconstructing major starformation episodes in galaxies. IKN is a faint dwarf spheroidal (dSph) in the M 81 group ... -
Photometric and structural properties of NGC 6544 : a combined VVV-Hubble Space Telescope study
(2014) [Artigo de periódico]We combine archival Hubble Space Telescope imaging with wide-field near-infrared photometry to study the neglected metal-poor Galactic globular cluster NGC 6544. A high spatial resolution map of differential reddening over ... -
The globular cluster NGC 6642 : evidence for a depleted mass function in a very old cluster
(2009) [Artigo de periódico]We present photometry for the globular cluster NGC6642 using the F606W and F814W filters with the Advanced Camera for Surveys in the Wide Field Channel (ACS/WFC) third generation camera on board of Hubble Space Telescope. ... -
The globular cluster system of the Coma cD galaxy NGC 4874 from Hubble Space Telescope ACS and WFC3/IR imaging
(2016) [Artigo de periódico]We present new Hubble Space Telescope (HST) optical and near-infrared (NIR) photometry of the rich globular cluster (GC) system NGC 4874, the cD galaxy in the core of the Coma cluster (Abell 1656). NGC 4874 was observed ... -
The overlooked potential of generalized linear models in astronomy – III. Bayesian negative binomial regression and globular cluster populations
(2015) [Artigo de periódico]In this paper, the third in a series illustrating the power of generalized linear models (GLMs) for the astronomical community, we elucidate the potential of the class of GLMs which handles count data. The size of a galaxy’s ... -
The tidal tails of NGC 2298
(2011) [Artigo de periódico]We present an implementation of the matched-filter technique to detect tidal tails of globular clusters. The method was tested using the Sloan Digital Sky Survey (SDSS) data for the globular cluster Palomar 5 revealing its ... -
Two reddened globular cluster projected close to the galactic center : Palomar 6 and Djorgovski 1
(1995) [Artigo de periódico]We present NTT V,I observations of Palomar 6 and Djorgovski 1, two obscured loose clusters in crowded fields. We derive a reddening of E(B - V) = 1.33 ± 0.10, a distance dʘ ≈ 8.9 kpc, and a metallicity of [Fe/H] ≈ -0.4 for ... -
VLT-UVES analysis of 5 giants in 47 Tucanae
(2005) [Artigo de periódico]High resolution spectra of 5 giants, including a horizontal branch star, of the metal-rich globular cluster 47 Tucanae were obtained with the UVES spectrograph at the 8m VLT UT2-Kueyen telescope. The atmospheric parameters ...