Infrared composition of the Large Magellanic Cloud

Abstract The evolution of galaxies and the history of star formation in the Universe are among the most important topics in today’s astrophysics. Especially, the role of small, irregular galaxies in the star-formation history of the Universe is not yet clear. Using the data from the AKARI IRC survey...

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Main Authors: M. Siudek, A. Pollo, T. T. Takeuchi, Y. Ita, D. Kato, T. Onaka
Format: Article
Language:English
Published: SpringerOpen 2013-03-01
Series:Earth, Planets and Space
Subjects:
Online Access:https://doi.org/10.5047/eps.2012.09.001
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author M. Siudek
A. Pollo
T. T. Takeuchi
Y. Ita
D. Kato
T. Onaka
author_facet M. Siudek
A. Pollo
T. T. Takeuchi
Y. Ita
D. Kato
T. Onaka
author_sort M. Siudek
collection DOAJ
description Abstract The evolution of galaxies and the history of star formation in the Universe are among the most important topics in today’s astrophysics. Especially, the role of small, irregular galaxies in the star-formation history of the Universe is not yet clear. Using the data from the AKARI IRC survey of the Large Magellanic Cloud at 3.2, 7, 11, 15, and 24 μm wavelengths, i.e., at the mid- and near-infrared, we have constructed a multiwavelength catalog containing data from a cross-correlation with a number of other databases at different wavelengths. We present the separation of different classes of stars in the LMC in color-color, and color-magnitude, diagrams, and analyze their contribution to the total LMC flux, related to point sources at different infrared wavelengths.
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spelling doaj.art-349d85ec4eae483682f91cf9c0ff279d2023-10-29T12:17:23ZengSpringerOpenEarth, Planets and Space1880-59812013-03-0165322927110.5047/eps.2012.09.001Infrared composition of the Large Magellanic CloudM. Siudek0A. Pollo1T. T. Takeuchi2Y. Ita3D. Kato4T. Onaka5Center for Theoretical Physics of the Polish Academy of SciencesCenter for Theoretical Physics of the Polish Academy of SciencesDivision of Particle and Astrophysical Science, Nagoya UniversityAstronomical Institute, Tohoku UniversityInstitute of Space and Astronautical Science, Japan Aerospace Exploration AgencyDepartment of Astronomy, The University of TokyoAbstract The evolution of galaxies and the history of star formation in the Universe are among the most important topics in today’s astrophysics. Especially, the role of small, irregular galaxies in the star-formation history of the Universe is not yet clear. Using the data from the AKARI IRC survey of the Large Magellanic Cloud at 3.2, 7, 11, 15, and 24 μm wavelengths, i.e., at the mid- and near-infrared, we have constructed a multiwavelength catalog containing data from a cross-correlation with a number of other databases at different wavelengths. We present the separation of different classes of stars in the LMC in color-color, and color-magnitude, diagrams, and analyze their contribution to the total LMC flux, related to point sources at different infrared wavelengths.https://doi.org/10.5047/eps.2012.09.001Large Magellanic Cloudsky surveysinfraredAKARI
spellingShingle M. Siudek
A. Pollo
T. T. Takeuchi
Y. Ita
D. Kato
T. Onaka
Infrared composition of the Large Magellanic Cloud
Earth, Planets and Space
Large Magellanic Cloud
sky surveys
infrared
AKARI
title Infrared composition of the Large Magellanic Cloud
title_full Infrared composition of the Large Magellanic Cloud
title_fullStr Infrared composition of the Large Magellanic Cloud
title_full_unstemmed Infrared composition of the Large Magellanic Cloud
title_short Infrared composition of the Large Magellanic Cloud
title_sort infrared composition of the large magellanic cloud
topic Large Magellanic Cloud
sky surveys
infrared
AKARI
url https://doi.org/10.5047/eps.2012.09.001
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AT apollo infraredcompositionofthelargemagellaniccloud
AT tttakeuchi infraredcompositionofthelargemagellaniccloud
AT yita infraredcompositionofthelargemagellaniccloud
AT dkato infraredcompositionofthelargemagellaniccloud
AT tonaka infraredcompositionofthelargemagellaniccloud