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   <subfield code="a">Rapid photometric and spectroscopic evolution of the young planetary nebula Hen 3-1357 and its central star SAO 244567</subfield>
   <subfield code="h">[Elektronische Daten]</subfield>
   <subfield code="c">[V. Arkhipova, N. Ikonnikova, A. Kniazev, Andry Rajoelimanana]</subfield>
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   <subfield code="a">We present the results of spectroscopic and photometric observations for the young compact planetary nebula Hen 3-1357 and its central star SAO 244567. High-resolution spectroscopy has allowed the expansion velocity of the nebula, V exp = 8.4 ± 1.5 km s−1, and the heliocentric velocity of the object, V r = +12.6 ± 1.7 km s−1, to be determined. The gas shell parameters (N e , T e ), the extinction in the Hβ line, and the O, N, Ne, Ar, S, Cl, He, and C abundances have been determined from low-resolution spectra taken in 1992 and 2011. We have found significant changes in the relative intensities of forbidden lines in the spectrum of Hen 3-1357 within the last 20 years: the low-excitation [O I], [O II], and [N II] lines became stronger relative to Hβ by a factor of ∼2, while the [O III] lines weakened by a factor of ∼ 2, suggesting a decrease in the excitation class of the nebula. The V-band photometry performed under the ASAS-3 program revealed a decline in the yearly mean brightness of SAO 244 567 from 2001 to 2009 by $$0_.^m 5$$ and rapid variability with an amplitude of a few tenths of a magnitude. Published observational data in a wide spectral range, from the near ultraviolet to the radio band, suggest an appreciable weakening of the flux from the star and the nebula.</subfield>
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   <subfield code="t">Astronomy Letters</subfield>
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