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J/A+AS/128/255      Proper motions in M 11                            (Su+ 1998)
================================================================================
Membership determination of stars using proper motions in the region
of the open cluster M11
       Su C.-G., Zhao J.-L., Tian K.-P.
      <Astron. Astrophys. Suppl. Ser. 128, 255 (1998)>
      =1998A&AS..128..255S      (SIMBAD/NED BibCode)
================================================================================
ADC_Keywords: Clusters, open ; Proper motions
Keywords: star cluster: open - star cluster: individual: M11 -
          proper motion: membership determination

Abstract:
    Relative proper motions of 872 stars in the open cluster M 11 region
    are reduced using 10 plate pairs taken over time baselines of 16~70
    years with the double astrograph telescope of Shanghai Observatory.
    The scale is 30"/mm. The plates were measured with the PDS machines in
    the Purple Mountain Observatory in Nanjing and the Institute of
    Technology and Communication in Luoyang, China. The average proper
    motion accuracy is about 1.1mas/yr with 85% of the data better than
    1mas/yr. Membership probabilities of 785 stars within 25' centred on M
    11 are determined based on their proper motions. The method used is
    suggested by Su et al. (1995AcApS..15..217S) with some improvements of
    Zhao & He (1990A&A...237...54Z), in which the space distribution and
    magnitude dependencies for cluster stars are taken into account. The
    results are significantly good. The total integrated membership
    probabilities for all these stars is 547 and the number of stars with
    probabilities higher than 0.7 is 541. It can be found after the
    membership determination that there exists mass segregation in M 11.
    Some comparisons and discussion are also given.

Objects:
    ----------------------------------------------------------
       RA   (2000)   DE       Designation(s)
    ----------------------------------------------------------
     18 51.1      -06 16      M 11 = NGC 6705
    ----------------------------------------------------------

File Summary:
--------------------------------------------------------------------------------
  FileName        Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
table4.dat         80      872   Relative proper motions and membership
                                  probabilities of stars in the M11 region
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table4.dat
--------------------------------------------------------------------------------
   Bytes Format    Units      Label    Explanations
--------------------------------------------------------------------------------
   1-  4  I4       ---         Star    Star number
       5  A1       ---       n_Star    [*] *: Reference star
   6- 10  I5       ---         NSP     ? Star number in the catalogue of
                                          McNamara, Pratt & Sanders
                                          (1977A&AS...27..117M)
  13- 18  F6.3     cm          Xpos    Measured coordinate in X (1)
  21- 26  F6.3     cm          Ypos    Measured coordinate in Y (1)
  29- 33  F5.2     mag         Vmag    V magnitude
  36- 40  F5.2     mag         Bmag    ? B magnitude
  43- 48  F6.3 10-2arcsec/yr   pmX     Relative proper motion in X
  51- 56  F6.3 10-2arcsec/yr   pmY     Relative proper motion in Y
  59- 63  F5.3 10-2arcsec/yr e_pmX     Uncertainty of proper motion in X
  66- 70  F5.3 10-2arcsec/yr e_pmY     Uncertainly of proper motion in Y
  73- 74  I2       ---         Nplate  Number of the plate pairs
  77- 80  F4.2     %           Member  ? Membership probability
--------------------------------------------------------------------------------
Note (1): 1 mm = 30"
--------------------------------------------------------------------------------

Acknowledgements: Tian Kaiping <tkp@center.shao.ac.cn>
================================================================================
(End)                                    Francois Ochsenbein [CDS]   15-Jul-1997

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