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Mostrando ítems 411-419 de 419
Integral field spectroscopy of HII region complexes. The outer disk of NGC 6946.
(Monthly Notices of the Royal Astronomical Society, 2010)
Clarifying the nature of the brightest submillimetre sources: interferometric imaging of LH850.02
(Monthly notices of the royal astronomical society, 2008)
Caracterização fotométrica de aglomerados estelares nas regiões W 31 e NGC 6334
(Universidade Federal de Santa MariaBrasilFísicaUFSMPrograma de Pós-Graduação em FísicaCentro de Ciências Naturais e Exatas, 2018-03-06)
Stellar clusters are groups of gravitationally bounded stars which were born from the same molecular
cloud. In their initial phase, they remain bounded to the cloud and are called embedded
clusters. These objects have ...
Multiwavelength study of the G345.5+1.5 region
(EDP Sciences, 2019-02)
Context. The star formation process requires the dust and gas present in the Milky Way to self-assemble into dense reservoirs ofneutral material where the new generation of stars will emerge. Star-forming regions are usually ...
Deep 1.1mm-wavelength imaging of the GOODS-S field by AzTEC/ASTE - I. Source catalogue and number counts
(Monthly Notices of the Royal Astronomical Society, 2010)
Deep 1.1mm-wavelength imaging of the GOODS-S field by AzTEC/ASTE - I. Source catalogue and number counts
(Monthly Notices of the Royal Astronomical Society, 2010)
Structural analysis of massive protoclusters formed from cloud collision
(Universidad de los AndesFísicaFacultad de CienciasDepartamento de Física, 2022-12-15)
The main processes that trigger the collapse and fragmentation of giant molecular clouds (GMCs) in star-forming regions are poorly understood. One of the proposed mechanisms for the formation of massive stellar clusters ...