Katalog der Deutschen Nationalbibliothek

Neuigkeiten Donnerstag, 11. September 2025: Die Deutsche Nationalbibliothek öffnet wegen eines Beschäftigtentreffens an beiden Standorten erst um 15 Uhr. Die Ausstellungen des Deutschen Buch- und Schriftmuseums sind von 10 bis 18 Uhr geöffnet. Die Ausstellungen des Deutschen Exilarchivs 1933-1945 sind von 9 bis 21:30 Uhr geöffnet. // Thursday, 11 September 2025: The German National Library will not open until 15:00 due to a staff meeting at both locations. The exhibitions of the German Museum of Books and Writing will open from 10:00 to 18:00. The exhibitions of the German Exile Archive 1933–1945 will be open from 9:00 to 21:30.
 
 

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Online Ressourcen
Link zu diesem Datensatz https://d-nb.info/102368330X
Art des Inhalts Hochschulschrift
Titel Combining X-ray and optical/NIR data to study GRBs and their host galaxies / Andrea Rossi. Gutachter: Artie P. Hatzes ; Ulrich Heber ; Giampaolo Piotto
Person(en) Rossi, Andrea (Verfasser)
Hatzes, Artie P. (Akademischer Betreuer)
Heber, Ulrich (Akademischer Betreuer)
Piotto, Giampaolo (Akademischer Betreuer)
Verlag Jena : Thüringer Universitäts- und Landesbibliothek Jena
Zeitliche Einordnung Erscheinungsdatum: 2012
Umfang/Format Online-Ressource
Andere Ausgabe(n) Erscheint auch als Druck-Ausgabe: Rossi, Andrea: Combining X-ray and optical, NIR data to study GRBs and their host galaxies
Hochschulschrift Jena, Friedrich-Schiller-Universität Jena, Diss., 2012
Persistent Identifier URN: urn:nbn:de:gbv:27-20120619-122254-0
URL http://www.db-thueringen.de/servlets/DocumentServlet?id=20577 (Verlag) (kostenfrei zugänglich)
Sprache(n) Englisch (eng)
Anmerkungen In: This thesis focuses on the topic of Gamma-Ray Bursts (GRBs), which is currently one of the most fascinating research fields in Astrophysics. Gamma-Ray Bursts are flashes of high-energy radiation which appear in the sky at random times from random directions. Briefly, from a few milliseconds to a few minutes, they outshine every other source of gamma-rays in the sky, and then they fade away. The current model to explain the large amount of energy released during a GRB is the fireball model. Within this framework, the energy is released in a short period of time by the collapse of the core of a massive star or the merger of two compact stellar objects. The collapse of this compact object ejects ultra-relativistic polar jets. The internal dissipation of energy within the jets leads to non-thermal high-energy emission, the GRB itself. The shock created from the deceleration of the relativistic outflow in the interstellar medium leads to a long-lasting transient, visible from X-rays to the radio band, called afterglow.
Schlagwörter Röntgenastronomie
DDC-Notation 522.6863 [DDC22ger]
Sachgruppe(n) 520 Astronomie, Kartographie

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