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Cited article:
M. Juvela , V.-M. Pelkonen , S. Porceddu
A&A, 505 2 (2009) 663-671
Published online: 2009-07-28
This article has been cited by the following article(s):
14 articles
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The dense cores and filamentary structure of the molecular cloud in Corona Australis: Herschel SPIRE and PACS observations from the Herschel Gould Belt Survey
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FILAMENTS IN SIMULATIONS OF MOLECULAR CLOUD FORMATION
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The degeneracy between dust colour temperature and spectral index
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MODELING DUST AND STARLIGHT IN GALAXIES OBSERVED BYSPITZERANDHERSCHEL: NGC 628 AND NGC 6946
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The degeneracy between the dust colour temperature and the spectral index
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A Corona Australis cloud filament seen in NIR scattered light
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Galactic cold cores
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Planckearly results. XXV. Thermal dust in nearby molecular clouds
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Observation of light echoes around very young stars
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