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J/A+AS/114/499    Spectral Atlas of P Cygni in range 4840-6760A (Markova+, 1995)
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P Cygni - spectral  atlas  with complete line identifications
in the wavelength range from  4840  to 6760 A
    Markova N., Zamanov R.
   <Astron. Astrophys. Suppl. Ser. 114, 499 (1995)>
   =1995A&AS..114..499M      (SIMBAD/NED BibCode)
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ADC_Keywords: Spectroscopy
Keywords: P Cygni - line: identification -  atlases

Description:
    Using the coude spectrograph of the NAO 2m RCC telescope at the
    Rhodope Mountains, Bulgaria, 11 spectra in the wavelength range from
    4840 to 6760A of P Cygni were obtained during the years 1981, 1983 and
    1985. By averaging these spectra we achieved a S/N-ratio of about 50.
    Here we present a spectral atlas with complete line identifications.
    Apart from the lines listed by de Groot (1969) many pure bright lines
    are identified. Most of them are lines of FeIII with high multiplet
    numbers and NII. Further emission lines are those of SiII multiplets
    2, 4 and 5. A new feature is SII spectrum in absorption and emission.
    In addition to the forbidden lines discovered by Stahl et al. (1991,
    1993) three new lines, [FeII19] {lambda}5159, [FeII18] {lambda}5273
    and [FeII34] {lambda}5477 are identified. The presence of some [TiII9]
    lines as well as the red lines of [NII1] is considered as quite
    probable.

Objects concerned:
    ----------------------------------------------------
       RA  (2000)  DE       Name(s)
    ----------------------------------------------------
    20 17 47.1 +38 01 59    P Cyg = HR 7763 = HD 193237
    ----------------------------------------------------

File Summary:
--------------------------------------------------------------------------------
  FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
table1             69      287   P Cygni spectrum - wavelengths and
                                 identifications
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Byte-by-byte Description of file: table1
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   Bytes Format  Units   Label    Explanations
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   2-  8  F7.2   0.1nm   LamObs     Observational wavelengths
      10  A1     ---   n_LamObs     [?] When "?" It's an uncertain feature
      13  A1     ---     Nat        [ea] Nature of the line (1)
      14  A1     ---   n_Nat        [)] When ')': This feature and the
                                    following are believed to be formed by
                                    the same line or lines
  17- 21  F5.2   0.1nm   LamLab     []? Laboratory wavelengths
      22  A1     ---   n_LamLab     [?] Uncertainty sign
  25- 35  A11    ---     Ion        Identification element
      36  A1     ---   n_Ion        [*] '*' marks the most important
                                    contributor to a blend
  41- 43  A3     ---     Remarks    Remarks (2)
  47- 48  A2     ---     Remarks2   Additional remarks (3)
  52- 53  A2     ---   n_ForbidLine [--] "--" marks  the  area  of  overlapping
                                    of forbidden and permitted line
  55- 68  A14    ---     ForbidLine Forbidden line identification
      69  A1     ---  n2_ForbitLine [?] ? = an uncertain identification
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Note (1): a= absorption
          e= emission
Note (2): new= newly identified line
          1= line observed by de Groot (1969)
          2= line observed by Stahl et al. (1993)
Note (3): IS= interstellar line
          bl= blend
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References:
   De Groot, M., 1969, Bull. Astron. Inst. Net., 20, 225 (1969BAN....20..225D)
   Stahl, O., Mandel, H., Wolf, B., =1993A&AS...99..167S
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(End)                                             Simona Mei [CDS]   25-Jul-1995

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