J/ApJ/672/930      Distant CO clouds in third galactic quadrant (Vazquez+, 2008)
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Spiral structure in the outer galactic disk. I. The third galactic quadrant.
    Vazquez R.A., May J., Carraro G., Bronfman L., Moitinho A., Baume G.
   <Astrophys. J., 672, 930-939 (2008)>
   =2008ApJ...672..930V
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ADC_Keywords: Clusters, open ; Molecular clouds
Keywords: Galaxy: disk - Galaxy: structure -
          open clusters and associations: general

Abstract:
    We combine optical and radio observations to trace the spiral
    structure in the third quadrant of the Milky Way. The optical
    observations consist of a large sample of young open clusters and
    associations, whereas the radio observations consist of a survey of
    nearby and distant clouds observed in CO. Both the optical and radio
    samples are the largest ones thus far presented in the literature. We
    use this unique material to analyze the behavior of interstellar
    extinction and to trace the detailed structure of the third Galactic
    quadrant (TGQ).

Description:
    This sample extension comes from an observing run conducted in Cerro
    Tololo with the 1.0m telescope on nights 2005 November 28-December 4.

File Summary:
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 FileName   Lrecl  Records   Explanations
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ReadMe         80        .   This file
table3.dat     34       46   Basic parameters of the new distant CO clouds
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Byte-by-byte Description of file: table3.dat
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   Bytes Format Units   Label     Explanations
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   1-  6  F6.2  deg     GLON      Galactic longitude (1)
   8- 12  F5.2  deg     GLAT      Galactic latitude (1)
  14- 19  F6.2  km/s    Vlrs      LSR velocity
  21- 26  F6.3  kpc     dist      Heliocentric distance
  28- 34  F7.1  pc      Z         Height above the plane
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Note (1): Sources identified as [VMC2008] GLLL.ll+B.bb in Simbad
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History:
    From electronic version of the journal
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(End)                                      Patricia Vannier [CDS]    07-Apr-2010
