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Module: Astrophysik: Fenster zum Kosmos

Sequence: Start

Branching Point: Windows to the Universe

Sequence: radio astronomy branch

Branching Point: Radioastronomy

Sequence: Effelsberg - tek

Slide: The Effelsberg Radiotelescope

Slide:

Slide: The moving telescope

Slide:

Slide: The Very Long Baseline Interferometry

Slide: VLBI Network

Slide:

Slide: The Arecibo Telescope

Slide: The Very Large Array

Sequence: mw-map

Slide: How does the Milky Way look if we observe it with a radiotelescope ?

Slide:

Slide:

Sequence: science_with_effi

Slide: Galaxy NGC 1052

Slide: Galaxy NGC 1052 observed from 1995 to 2001

Slide: Quasar 3C273

Slide: The Quasar 3C273 and the jet

Slide: Quasar 3C273 observed from 1995 to 2001

Slide: Quasar 3C279

Slide: Quasar 3C279: the jet changes direction

Sequence: SN1993

Slide: Galaxy M81

Slide: The explosion

Slide: SuperNova 1993J

Slide: SuperNova 1993J

Sequence: neutrinos

Slide: Neutrinos ...

Slide: AMANDA, a neutrino telescope within the South Polar ice shield, ...

Slide: Probe of the AMANDA neutrino telescope

Slide: Principle model of the AMANDA telescope

Slide: Cerenkov radiation ...

Slide: If the light cone of a myon ...

Slide: Neutrino astronomy is an adventure:

Slide: Probe of the AMANDA successor IceCube

Forward

How does the Milky Way look if we observe it with a radiotelescope ?

The whole Milky Way has been observed with Effelsberg Radiotelescope, at a wavelength of 11 centimetres.

Next animations show the radio map of the Milky Way: the red central spot where the movie slows down corresponds to the galactic centre.

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