File:Light curve of AKO 9 in 47 Tucanae (eso9703b).jpg

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Light_curve_of_AKO_9_in_47_Tucanae_(eso9703b).jpg (771 × 554 pixels, file size: 51 KB, MIME type: image/jpeg)

Captions

Captions

In this diagramme are shown the light curves (change of light intensity with time) for the binary system AKO 9 (o) and two other stars (x) with constant brightness in the southern globular cluster 47 Tucanae.

Summary

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Description
English: In this diagramme are shown the light curves (change of light intensity with time) for the binary system AKO 9 (o) and two other stars (x) with constant brightness in the southern globular cluster 47 Tucanae.

The ultraviolet magnitude of AKO 9 was U ~ 18 at the time of the first observation. The subsequent rise was very fast: 2.1 magnitudes in 1 hour. It then remained constant for about 2 hours before increasing by another 0.5 mag.

The observations ended with the system in this bright state. It is not known if and when it reverted to its normal state. At the end of these observations, AKO 9 was the brightest ultraviolet source in the core of the cluster.
Date 15 January 1997 (upload date)
Source
This media was produced by the European Southern Observatory (ESO), under the identifier eso9703b

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Author ESO
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current20:41, 22 June 2024Thumbnail for version as of 20:41, 22 June 2024771 × 554 (51 KB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://www.eso.org/public/archives/images/large/eso9703b.jpg via Commons:Spacemedia

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