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ADCADC/CDS Standard Document for Catalog:
/catalogs/2/2055/

The following is the "ReadMe" document that describes this ADC catalog. You can access the files described here in three ways:

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2. Get the data files via anonymous FTP. (See Note.) [ftp


II/55               Gershberg Flare Star Catalogue   (Shakhovskaya 1971)
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Gershberg Flare Star Catalogue
     Shakhovskaya N.I.
    <Veroeff. Bamberg IX, 138 (1971)>
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ADC_Keywords: Stars, flare

Description:
    This catalog groups the flare stars as presented in the IAU Colloquium
    15 (combined Colloquium of Commisions 27 and 42) held at Bamberg
    31-Aug to 03-Sep 1971 entitled
    "New Directions and New Frontiers in Variable Star Research"

    The following definition of the UV Cet-type variables was given in
    Kukarkin's General Catalogue of Variable Stars (1969): "dMe stars,
    sometimes subject to flares with the amplitude from 1 to 6mag. Maximum
    brightness is attained in seconds or dozens of seconds after the
    commencement of the flare; the star returns to its normal brightness
    after several minutes, or dozens of minutes. A typical representative
    is UV Ceti." Now it is impossible to consider this definition as a
    quite right because: 1) There are a number of M-dwarf stars affected
    by the flares similar to the UV Ceti flares, but in their quiet state
    spectra, no emission lines are observed. For example, BD+43 44A, BD+43
    44 B, and SZ UMa, the flare activity of these stars were detected in
    Crimea; and probably BD-04 4048B is suspected as a flare star by
    HERBIG. 2) The lower limit of flare amplitude cited in Kukarkin's
    corresponds to visual observations, but the modern photoelectric
    observations register flares with amplitudes to 0.02-0.05mag.
    Therefore we suppose, that UV Cet-type variables are K-M dwarfs, which
    show quick flares with amplitudes exceeding the observational errors,
    and duration of the flares are from a few seconds up to a few hundred
    minutes.

    The "catalog" file includes only such variable K-M dwarf stars, for
    which existing observations allow to construct flare light curves. All
    stars in "catalog", except V371 Ori, have photoelectric flare light
    curves. The strong flare of V371 Ori was observed in radio region, but
    simultaneous optical observations were carried out photographically
    and visually only.

File Summary:
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 FileName    Lrecl    Records    Explanations
--------------------------------------------------------------------------------
ReadMe          80          .    This file
catalog.dat     69         53    The catalogue of flare stars
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Byte-by-byte Description of file: catalog.dat
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   Bytes Format  Units   Label    Explanations
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   1- 10  A10    ---     Name     Designation of the object
  12- 19  F8.4   deg     RAdeg    Right ascension B1950 (degrees)
  21- 28  F8.4   deg     DEdeg    Declination B1950 (degrees)
  31- 38  A8     ---     Rem      Remark (Multiplicity, other id., etc.)
  41- 50  F10.5  ---     Period   []? Period (for binaries) in days or
                                    years depending on x_Period
      51  A1     ---     x_Period [YD] Units in which Period is expressed
  54- 58  F5.2   arcsec  MajAxis  []?  Semi-major axis (for binaries)
  61- 69  A9     ---     Remark   Other designation (Gliese number) or comment
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Historical Notes:
 * The tape was provided by Bamberg Observatory to CDS in 1978
 * 09-Oct-1995: catalogue reformatted at CDS
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(End)                                          Joseph Florsch [CDS]  09-Oct-1995

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