Navegação por Assunto "Nuvens de magalhaes"
Resultados 21-29 de 29
-
Spectral evolution of star clusters in the Large Magellanic Cloud : I. blue concentrated clusters in the range 40-300 Myr
(2006) [Artigo de periódico]Aims. Integrated spectroscopy of a sample of 17 blue concentrated Large Magellanic Cloud (LMC) clusters is presented and its spectral evolution studied. The spectra span the range ≈(3600−6800) Å with a resolution of ≈14Å ... -
Star formation in distant starburst galaxies
(2000) [Artigo de periódico]This paper discusses the stellar population content of distant (5 000kms−1 VR 16 000kms−1) galaxies with enhanced star-formation activity. Distinction is made between isolated galaxies and galaxies morphologically disturbed, ... -
Structures in surface-brightness profiles of LMC and SMC star clusters : evidence of mergers?
(2008) [Artigo de periódico]Context. The LMC and SMC are rich in binary star clusters, and some mergers are expected. It is thus important to characterise single clusters, binary clusters and candidates for mergers. Aims. We selected a sample of star ... -
The VISCACHA survey : III. Star clusters counterpart of the Magellanic Bridge and Counter-Bridge in 8D
(2021) [Artigo de periódico]Context. The interactions between the Small and Large Magellanic Clouds (SMC and LMC) created the Magellanic Bridge; a stream of gas and stars pulled out of the SMC towards the LMC about 150 Myr ago. The tidal counterpart ... -
The VISCACHA survey : II. Structure of star clusters in the Magellanic clouds periphery
(2020) [Artigo de periódico]We provide a homogeneous set of structural parameters of 83 star clusters located at the periphery of the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC). The clusters’ stellar density and surface brightness ... -
The VISCACHA survey : I. Overview and first results
(2019) [Artigo de periódico]The VISCACHA(VIsible Soar photometry of star Clusters in tApii and Coxi HuguA) Survey is an ongoing project based on deep photometric observations of Magellanic Cloud star clusters, collected using the SOuthern Astrophysical ... -
The VISCACHA survey : IV. The SMC West Halo in 8D
(2022) [Artigo de periódico]The structure of the Small Magellanic Cloud (SMC) is very complex, in particular in the periphery that suffers more from the interactions with the Large Magellanic Cloud (LMC). A wealth of observational evidence has been ... -
The VISCACHA survey : VIII. Chemical evolution history of the small Magellanic cloud west halo clusters
(2023) [Artigo de periódico]The chemical evolution history of the Small Magellanic Cloud (SMC) has been a matter of debate for decades. The challenges in understanding the SMC chemical evolution are related to a very slow star formation rate (SFR) ... -
The VISCACHA survey : V. Rejuvenating three faint SMC clusters
(2022) [Artigo de periódico]We present the analysis of three faint clusters of the Small Magellanic Cloud RZ 82, HW 42, and RZ 158. We employed the SOAR telescope instrument SAM with adaptive optics, allowing us to reach to V ∼ 23–24 mag, unprecedentedly, ...