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J/PAZh/38/183 IRAS 19336-0400 UBV light curves (Arkhipova+, 2012)
Variability of hot supergiant IRAS 19336-0400 in the early phase of planetary nebula ionization. Arkhipova V.P., Burlak M.A., Esipov V.F., Ikonnikova N.P., Komissarova G.V. <Pis'ma Astron. Zh. 38, 183 (2012)> =2012PAZh...38..183A =2012AstL...38..157A
ADC_Keywords: Stars, supergiant ; Photometry, UBV Keywords: proto-planetary nebulae - photometric and spectral observations - light variability Abstract: We present photoelectric and spectral observations of a hot candidate proto-planetary nebula early B-type supergiant with emission lines in spectrum-IRAS 19336-0400. The light and color curves display fast irregular brightness variations with maximum amplitudes {Detla}V=0.30m, {Detla}B=0.35m, {Detla}U=0.40m and color-brightness correlations. By the variability characteristics IRAS 19336-0400 appears similar to other hot proto-planetary nebulae Description: In 2006 we started systematic photometric observations of IRAS 19336-0400. Measurements were carried out on the 60-cm telescope Zeiss-1 at SAI Crimean Station with the use of photoelectric UBV photometer constructed by Lyuty (1971, Soobshch. GAISh 172, 30). Objects: --------------------------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------------------------- 19 36 17.52 -03 53 25.3 IRAS 19336-0400 = PN G034.5-11.7 --------------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 24 155 UBV observations of IRAS 19336-0400 in 2006-2011
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 7 I7 d JD Julian date 9- 13 F5.2 mag Vmag V magnitude 15- 18 F4.2 mag B-V B-V colour index 20- 24 F5.2 mag U-B U-B colour index
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 18-Apr-2012
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