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LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas
Article . 2019
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Full-Text: https://www.researchgate.net/publication/230978900_Infrared_Dark_Clouds_in_the_Small_Magellanic_Cloud
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LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas
Article . 2020
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Full-Text: https://doi.org/10.1088/0004-6256/138/4/1101
Data sources: LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas
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Infrared dark clouds in the small magellanic cloud?

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 2009 English
Authors: Lee, M. Y.; Jones, P. A.;

handle: 10533/239504 , 10533/237030

Infrared dark clouds in the small magellanic cloud?

Abstract

We have applied the unsharp-masking technique to the 24 μm image of the Small Magellanic Cloud (SMC), obtained with the Spitzer Space Telescope, to search for high-extinction regions. This technique has been used to locate very dense and cold interstellar

CENASTRO

FONDAP

WOS

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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