J/ApJ/640/982         43GHz SiO maser features around VX Sgr       (Chen+, 2006)
Inward motions of the compact SiO masers around VX Sagittarii.
    Chen X., Shen Z.-Q., Imai H., Kamohara R.
   <Astrophys. J., 640, 982-994 (2006)>
   =2006ApJ...640..982C 2006ApJ...640..982C
ADC_Keywords: Masers
Keywords: circumstellar matter - masers - stars: individual (VX Sagittarii) -
          stars: kinematics
Abstract:
    We report Very Long Baseline Array (VLBA) observations of 43GHz v=1,
    J=1-0 SiO masers in the circumstellar envelope of the M-type
    semiregular variable star VX Sgr at three epochs during 1999
    April-May. These high-resolution VLBA images reveal a persistent
    ringlike distribution of SiO masers with a projected radius of ∼3
    stellar radii. The typical angular size of 0.5mas for individual maser
    features was estimated from two-point correlation function analysis of
    maser spots.
Description:
    The 43GHz v=1, J=1-0 SiO maser emission toward VX Sgr was observed at
    three epochs (1999 April 24, May 23, and May 31) using the Very Long
    Baseline Array (VLBA) of the NRAO.
Objects:
    --------------------------------------------------
       RA   (2000)   DE      Designation(s)
    --------------------------------------------------
    18 08 04.0   -22 13 27   VX Sagittarii = V* VX Sgr
    --------------------------------------------------
File Summary:
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 FileName   Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe         80        .   This file
table2.dat     86      110   43GHz SiO maser features around VX Sgr
                              observed by the VLBA on 1999 April 24 (Epoch 1)
table3.dat     86      110   43GHz SiO maser features around VX Sgr
                              observed by the VLBA on 1999 May 23 (Epoch 2)
table4.dat     86      105   43GHz SiO maser features around VX Sgr
                              observed by the VLBA on 1999 May 31 (Epoch 3)
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See also:
  J/A+A/393/115 : 86GHz SiO maser survey of late-type stars (Messineo+, 2002)
  J/A+A/418/103 : 86GHz SiO maser survey in the Inner Galaxy (Messineo+, 2004)
  J/A+A/435/575 : 86GHz SiO maser survey of late-type stars III (Messineo+ 2005)
Byte-by-byte Description of file: table2.dat table3.dat table4.dat
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   Bytes Format Units     Label      Explanations
--------------------------------------------------------------------------------
   1-  3  I3    ---       Seq        Sequential number (1)
       4  A1    ---     n_Seq        [ab] Note on Seq (2)
   6- 10  F5.2  km/s      VLSR       Velocity in the Local Standard of Rest
                                      at the peak of the velocity profile
  12- 15  F4.2  km/s    e_VLSR       Error in VLSR
  17- 20  F4.2  km/s      Delu       Velocity range across the feature (3)
  22- 25  F4.2  km/s      DelV       FWHM velocity ΔV
  27- 30  F4.2  km/s    e_DelV       Error on DelV
  32- 38  F7.3  mas       x          Feature position in Right Ascension (4)
  40- 44  F5.3  mas     e_x          Error on x (4)
  46- 52  F7.3  mas       y          Feature position in Declination (4)
  54- 58  F5.3  mas     e_y          Error on y (4)
  60- 63  F4.2  mas       L          Angular size of the feature
  65- 68  F4.1  Jy        Sp         Peak flux density (43GHz) of the feature
  70- 74  F5.1  Jy.km/s   Sint       Integrated flux density of all spots
                                      in the feature
  76- 78  I3    ---       ID1        ? Match ID at epoch 1
  80- 82  I3    ---       ID2        ? Match ID at epoch 2
  84- 86  I3    ---       ID3        ? Match ID at epoch 3
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Note (1): Seq corresponds to ID1 in table 2 ([CSI2006] 1 NNN in Simbad),
           ID2 in table 3 ([CSI2006] 2 NNN in Simbad), and
           ID3 in table 4 ([CSI2006] 3 NNN in Simbad).
Note (2): Note on Seq, defined as follows:
    a = Feature that cannot be well represented by a Gaussian curve
    b = Reference feature
Note (3): Δu is defined as the difference between the maximal and
           minimal velocities of the spots in the feature.
Note (4): Feature positions (x, y) in Right Ascension and Declination were
     determined from an intensity-weighted average over maser spots in 
     the feature. The uncertainty (σx, σy) of a feature
     position was defined as the square root of the squared sum of the
     mean spot distance from the defined feature position and the mean
     measurement error of the spot positions. The weights proportional to
     the intensity of the spot were applied in the uncertainty estimation.
     The typical position uncertainties of the features are 0.01 and
     0.02mas for Right Ascension and Declination, respectively. The
     positions are measured with respect to the reference feature at (0,0).
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History:
    From electronic version of the journal
(End)                                       Marianne Brouty [CDS]    14-Aug-2007