Near-infrared flare from Galactic Centre (lightcurve)

This image displays the "light curve" of a light flare from the galactic centre, as observed in the K-band (wavelength 2.2 µm) on June 16, 2003. This and a second flare discovered about 24 hours earlier show variability on a time scale of a few minutes and appear to show larger variations (arrows) with a 17-minute periodicity. The rapid variability implies that the infrared emission comes from just outside (the event horizon of) the black hole. If the periodicity is a fundamental property of the motion of gas orbiting the black hole, the Galactic Centre black hole must rotate with about half the maximum spin rate allowed by General Relativity. The present observations thus probe the space-time structure in the immediate vicinity of that event horizon.

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ESO

Om bilden

ID:eso0330b
Typ:Diagram
Publiceringsdatum:29 oktober 2003
Relaterade pressmeddelanden:eso0330
Storlek:800 x 906 px

Om objektet

Namn:Milky Way Galactic Centre
Typ:Milky Way : Galaxy : Component : Center/Core
Avstånd:25000 ljusår
Kategori:Galaxies

Bildformat

Originalstorlek
215,4 kB
Stor jpeg
98,7 kB
Skärmstor jpeg
120,0 kB

Skrivbordsunderlägg

1024x768
84,7 kB
1280x1024
110,7 kB
1600x1200
138,1 kB
1920x1200
152,5 kB
2048x1536
181,9 kB

Färger och filter

BandVåglängdTeleskop
Infrarött
K
2.2 μmVery Large Telescope

Exposure time: 600s