J/PAZh/32/737    UBV light curve and spectroscopy of StHa62   (Arkhipova+, 2006)
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Spectroscopy and photometry of the protoplanetary nebula candidate
StHa62 = IRAS 07171+1823.
    Arkhipova V.P., Klochkova V.G., Chentsov E.L., Esipov V.F., Ikonnikova N.P.,
    Komissarova G.V.
   <Pis'ma Astron. Zh. 32, 737 (2006)>
   =2006PAZh...32..737A
   =2006AstL...32..661A
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ADC_Keywords: Planetary nebulae; Photometry, UBV; Spectroscopy

Abstract:
    Photoelectric observations of HD 51585 (OY Gem), a B[e] star with an
    infrared excess and a candidate for protoplanetary nebulae, obtained
    with a 60-cm telescope at the Crimean Station of Sternberg
    Astronomical Institute in 1992-2005 are presented. The star exhibited
    rapid irregular brightness variations with amplitudes from 0.1mag in
    the V band to 0.2mag in the U band within the observing season as
    well as slow systematic variations. with a quasi-period of ~2800-days.
    Low-resolution spectroscopy performed in 1994-2005 has revealed
    significant variability of the Balmer and Paschen hydrogen emission
    lines as well as the HeI and OI lines. Equivalent widths are given for
    the HI, HeI, OI, and FeII lines. Correlation has been found between
    the star's photometric variability and the hydrogen line intensities.

Objects:
    -------------------------------------------------------------------------
       RA   (2000)   DE       Designation(s)
    -------------------------------------------------------------------------
    07 20 01.614 +18 17 26.47 StHA 62 = PN G199.4+14.3 = IRAS 07171+1823
    -------------------------------------------------------------------------

File Summary:
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 FileName   Lrecl  Records   Explanations
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ReadMe         80        .   This file
table3.dat     61       48   Parameters of individual lines in the spectrum
                              of StHa62
table7.dat     42       50   UBV observations of StHa62
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See also:
   J/A+A/385/884 : BVRIJHK photometry of 27 post-AGB candidates (Fujii+, 2002)

Byte-by-byte Description of file: table3.dat
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   Bytes Format Units   Label    Explanations
--------------------------------------------------------------------------------
   1-  8  A8    ---     El       ? Element
       9  A1    ---   n_El       Note to Element (1)
  10- 12  A3    ---     Rem      Remarks to observed parameters
  15- 21  F7.2  0.1nm   Lambda   Wavelength
  23- 27  F5.2  ---     r1999    ? Residual intensity of Mar. 6 1999 observation
      28  A1    ---   u_r1999    Uncertainty flag on r1999
      29  A1    ---   n_r1999    [#] Saturated line
  31- 33  I3    km/s    Vr1999   ? Heliocentric radial velocity of
                                    Mar.6 1999 observation
      34  A1    ---   u_Vr1999   ? Uncertainty flag on Vr1999
  37- 42  F6.3  ---     r2000    ? Residual intensity of Apr.23 2000 observation
      43  A1    ---   u_r2000    Uncertainty flag on r2000
      44  A1    ---   n_r2000    [#] Saturated line
  46- 47  I2    km/s    Vr2000   ? Heliocentric radial velocity of
                                    Apr.23 2000 observation
      48  A1    ---   u_Vr2000   Uncertainty flag on Vr2000
  51- 55  F5.2  ---     r2002    ? Residual intensity of Dec. 2 2002 observation
      56  A1    ---   u_r2002    Uncertainty flag on r2002
  59- 60  I2    km/s    Vr2002   ? Heliocentric radial velocity of
                                    Dec.2 2002 observation
      61  A1    ---   u_Vr2002   Uncertainty flag on Vr2002
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Note (1): Notes as follows:
     *  = profile of P Cyg
    min = minimal values of parameters
    max = maximal values of parameters
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Byte-by-byte Description of file: table7.dat
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   Bytes Format Units   Label     Explanations
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   1-  7  I7    d       JD        Julian date
   9- 14  F6.3  mag     Umag      U magnitude
  16- 21  F6.3  mag     Bmag      B magnitude
  23- 28  F6.3  mag     Vmag      V magnitude
  30- 35  F6.3  mag     U-B       U-B color index
  37- 42  F6.3  mag     B-V       B-V color index
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(End)                            Veta Avedisova [INASAN]             11-Apr-2007
