Studies of the Hot Interstellar Medium in the Large Magellanic Cloud

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dc.contributor.advisor Sasaki, Manami (Dr.) Warth, Gabriele 2014-12-16T08:50:48Z 2014-12-16T08:50:48Z 2014
dc.identifier.other 423511092 de_DE
dc.identifier.uri de_DE
dc.description.abstract The hot interstellar medium (ISM) is defined as the plasma which can be found between the stars of a galaxy and has a temperature of 10^6 – 10^7 K. Within the scope of this thesis, the hot ISM of the supergiant shell LMC-SGS 2 and the HII region DEM L299 in the Large Magellanic Cloud have been studied. It was shown that DEM L299 harbors not only the supernova remnant SNR B0543-68.9 in projection, as believed up to now, but also a superbubble. A multi-frequency morphological study was performed in X-ray, optical, and radio wavelengths in order to study the distribution of the hot, the warm, and the cold ISM of this region. In addition, an X-ray spectral analysis has been performed for LMC-SGS 2, SNR B0543-68.9, the DEM L299 superbubble, and the superbubble blowout. en
dc.language.iso en de_DE
dc.publisher Universität Tübingen de_DE
dc.rights ubt-podok de_DE
dc.rights.uri de_DE
dc.rights.uri en
dc.subject.classification Astronomie , Interstellare Materie , Astrophysik , Astronomie , Astrophysik , Interstellare Materie de_DE
dc.subject.ddc 520 de_DE
dc.subject.ddc 530 de_DE
dc.subject.other supernova remnant en
dc.subject.other Superbubble de_DE
dc.subject.other Supergiant Shell de_DE
dc.subject.other Supernova Überrest de_DE
dc.title Studies of the Hot Interstellar Medium in the Large Magellanic Cloud en
dc.type Dissertation de_DE
dcterms.dateAccepted 2014-12-10
utue.publikation.fachbereich Mathematisch-Naturwissenschaftliche Fakultät de_DE
utue.publikation.fakultaet 7 Mathematisch-Naturwissenschaftliche Fakultät de_DE


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