Scene

Module Menu

Module: Astrophysik: Schwarze Loecher

Sequence: Start

Slide:

Slide: Black Holes

Branching Point: Identification of Black Holes

Sequence: our own BH

Slide: The Milky Way Center

Slide: Movement of Stars in the Milky Way Centre

Slide: Kepler Ellipses around Sagittarius A*

Slide: S2, a Star in Narrow Orbit Around the Black Hole

Slide: S2 in its Orbit

Slide: Flares From Sagittarius A*

Sequence: sharp_ir

Slide: The NTT Telescope

Slide: The Speckle Camera SHARP I

Slide: Optical System of SHARP I

Slide: The Speckle Method

Slide:

Sequence: xmm_newton

Slide: XMM-Newton Satellite

Slide: Where is XMM-Newton now?

Slide: EPIC Camera

Slide: EPIC-pn CCD

Slide: Image Taken With XMM-Newton

Slide: Geminga, a Neutron Star

Slide: Geminga as a Magnet

Sequence: Biographie 31410: John Archibald Wheeler

Slide: J. A. Wheeler: The Inventor of the Name "Black Hole"

Sequence: Kinder: Schwarze Lcher

Slide:

Back

Forward

The Speckle Method

Speckle imaging involves taking hundreds or thousands of short exposure images, and the later reconstruction of a sharp image with the aid of a computer.

Between spring 1992 and summer 2002 Speckle-Camera SHARP I observed the very central region of the Milky Way.

[ Sitemap ] [ info ] This website was created by the MPI for the History of Science.