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Optical photometry of V4334 Sgr (Sakurai's Object)

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Abstract

The optical photometric evolution of the final helium flash object V4334 Sgr from 1994 to 2001 is described. The rise to optical maximum (1994–1996) is characterized by a continuous increase of colour indices, indicating a slowly expanding, cooling pseudo-photosphere. This photosphere became stationary in 1997. In the following years, the object underwent brightnessdeclines of increasing strength, which are similar in character to the `reddeclines' of RCB stars. The fading of V4334 Sgr is more dramatic than anybrightness decline of an RCB star: at present, only 10-5 of the visual light reaches the observer. Most short-wavelength radiation is absorbed by a dust envelopethat completely surrounds the star, and is re-radiated in the infrared. The sparse optical data of 2000–2001 show that the obscuration has not increased in strength any more. The light curve of V4334 Sgr is similar to that of the final helium flash object V605 Aql which erupted in 1919.

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  1. WE/OBSS, Vrije Universiteit Brussel, Pleinlaan 2, B-1050, Brussel, Belgium

    Hilmar W. Duerbeck

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  1. Hilmar W. Duerbeck
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Duerbeck, H.W. Optical photometry of V4334 Sgr (Sakurai's Object). Astrophysics and Space Science 279, 5–14 (2002). https://doi.org/10.1023/A:1014627418565

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