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Download "Zukunft der Röntgenastronomie - Jörn Wilms bei #FasziAstroOnline"

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Table of contents
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Table of contents

0:00
Begrüßung
8:00
Was ist Rosetta?
9:35
Die erste E-Rosetta-Himmelsdurchmusterung
13:30
Die Milchstraße
13:53
Das Galaktische Zentrum
15:32
Das Andromeda Nebel
17:40
Galaxienhaufen
18:46
Struktur des Universums
26:14
Was kann Athena?
28:07
Bilder von Athena
29:43
Fazit
33:01
Wie lässt sich herausfinden, ob Doppelsterne aus Neutronensternen stammen?
34:33
In schwarze Löcher im Radio und Röntgenbereich sichtbar oder nur durch Gamma Ray Burst bzw. Irritierende Gas?
35:46
Wie ändert sich die Helligkeit von Galaxienhaufen?
36:54
Früheres Supermassives Schwarzes Loch?
38:53
Hobby Radioastronomie
41:23
Widefield Imaging
43:20
Wie bricht ein Satellit auseinander?
45:19
Wie funktionieren Röntgenspiegel?
51:15
Was ist die bedeutendste Entdeckung der Astronomie?
53:53
Wie kann es sein, dass das Galaktische Zentrum Röntgenstrahlung emittiert, wenn doch das Schwarze Loch gerade nicht aktiv ist?
56:52
Wie und warum wurde das Material gewählt?
Video tags
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Video tags

Astronomie
Röntgenstrahlung
Röntgenastronomie
Chandra
XMM-Newton
XMM
eROSITA
Athena
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Description:

Faszination Astronomie Online bietet euch immer dienstags und donnerstags an dieser Stelle um 19 Uhr eine halbe Stunde Astronomie. Die Röntgenastronomie hat in den letzten 30 Jahren ein völlig neues Bild des heißen Universums geliefert. Der Vortrag wird einen Überblick über diese Ergebnisse geben und die geplante weitere Entwicklung des Feldes darstellen, insbesondere auch über die Planungen zum nächsten Großprojekt der Röntgenastronomie, der Athena-Mission. Jörn Wilms ist Professor für Astronomie und Astrophysik an der Dr. Karl Remeis-Sternwarte, dem Astronomischen Institut der Friedrich-Alexander-Universität Erlangen-Nürnberg

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