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Autor:
Annika Franeck, Richard Wünsch, Sergio Martínez-González, Ivana Orlitová, Peter Boorman, Jiří Svoboda, Dorottya Szécsi, Vanesa Douna
Inspired by the excess soft X-ray emission recently detected in Green Pea galaxies, we model the soft X-ray emission (0.5 - 2.0 keV) of hot gas from star cluster winds. By combining individual star clusters, we estimate the soft X-ray emission expect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a978557135460e1248a8b34e53a253c8
