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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Format: | Article |
Language: | English |
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SpringerOpen
2013-03-01
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Series: | Earth, Planets and Space |
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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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format | Article |
id | doaj.art-349d85ec4eae483682f91cf9c0ff279d |
institution | Directory Open Access Journal |
issn | 1880-5981 |
language | English |
last_indexed | 2024-03-11T15:15:37Z |
publishDate | 2013-03-01 |
publisher | SpringerOpen |
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series | Earth, Planets and Space |
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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