First study of the supernova remnant population in the Large Magellanic Cloud with eROSITA
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Le résumé fourni par la source
Aims. Supernova remnants (SNRs) are responsible for the injection of energy and chemical elements into the interstellar medium (ISM). The emission from SNRs can be studied to infer information about the supernova (SN) explosion itself as well as about the properties of the surrounding ISM. Studying a sample of SNRs in a galaxy provides an opportunity to better understand stellar feedback, and the best laboratory for such an investigation is the Large Magellanic Cloud (LMC). The LMC is the nearest star-forming galaxy, it lies outside the Galactic plane line of sight, and therefore its foreground absorption is low. Methods. The eROSITA telescopes are the best instruments currently available to perform a survey of the SNRs in the entire LMC due to their large field of view and their high sensitivity towards soft X-rays. We used the sample of SNRs reported in the previous paper and performed a spectral analysis on a part of the sample. We estimated the flux and the luminosity of the fainter sources using the energy conversion factor obtained assuming a non-equilibrium ionisation plasma model. Results. The X-ray luminosity function (XLF) of SNRs in the LMC shows a relatively large number of SNRs at high luminosities. We fitted the distribution with two Gaussian components, which yielded best-fit maxima for the L X [0.3-8.0keV] distribution at m 1 = 10 34.7±0.2 erg s −1 and m 2 = 10 36.5±0.4 erg s −1 . We compared the XLF of the LMC with the XLFs of the Small Magellanic Cloud (SMC), M31, and M33 using a power-law fit and an Anderson-Darling (DA) test. The power indices of the XLFs of the LMC and SMC appear consistent with each other, while those of M33 and M31 are larger. Thus, the latter have steeper power laws, indicating a lower number of X-ray luminous SNRs with respect to the Magellanic Clouds. The DA test showed that the luminosity distributions of SNRs in the SMC and LMC are compatible with being extracted from the same underlying distribution. They are also compatible for different galaxies if we consider the same lower limit for L X [0.3-8.0 keV] for the entire distribution. Finally, we compared the luminosity and the X-ray sizes (diameter) of the SNRs in our sample. We observed a general trend of anti-correlation between size and X-ray luminosity that can be interpreted as a result of fading with time.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Le contrôle bibliographique ouvert
DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.
- Titre Crossref
- First study of the supernova remnant population in the Large Magellanic Cloud with eROSITA
- Date Crossref
- 01/05/2026
- Éditeur
- EDP Sciences
- Type
- journal-article
Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.
Où se fait cette recherche
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Friedrich-Alexander-Universität Erlangen-Nürnberg pays non établi dans la noticeUniversité ou école supérieure
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Space Telescope Science Institute pays non établi dans la noticeStructure de recherche
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Observatoire astronomique de Strasbourg pays non établi dans la noticeStructure de recherche
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Western Sydney University pays non établi dans la noticeUniversité ou école supérieure
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Max Planck Institute for Extraterrestrial Physics pays non établi dans la noticeStructure de recherche
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National University of Ireland pays non établi dans la noticeUniversité ou école supérieure
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Australia Telescope National Facility pays non établi dans la noticeStructure de recherche
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Cerro Tololo Inter-American Observatory pays non établi dans la noticeStructure de recherche
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The University of Western Australia International Centre for Radio Astronomy Research (ICRAR) pays non établi dans la noticeUniversité ou école supérieure
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International Centre for Radio Astronomy Research pays non établi dans la noticeInstitution
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Universität Hamburg pays non établi dans la noticeUniversité ou école supérieure
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Dr. Karl Remeis Observatory pays non établi dans la noticeInstitution
Friedrich-Alexander-Universität Erlangen-Nürnberg, Space Telescope Science Institute et Observatoire astronomique de Strasbourg, avec 9 autres affiliations.
Une affiliation ne permet pas de déduire la nationalité d’un auteur.