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J/ApJS/136/463     Distances and metallicities of HVCs and IVCs   (Wakker, 2001)
================================================================================
Distances and metallicities of high- and intermediate-velocity clouds.
    Wakker B.P.
   <Astrophys. J. Suppl. Ser. 136, 463 (2001)>
   =2001ApJS..136..463W
================================================================================
ADC_Keywords: Molecular clouds ; Abundances ; Stars, distances
Keywords: Galaxy: halo - SM: abundances - ISM: clouds - ISM: structure -
          radio lines: ISM - ultraviolet: ISM

Description:
    A table is presented that summarizes published absorption line
    measurements for the high- and intermediate-velocity clouds (HVCs and
    IVCs). New values are derived for N(HI) in the direction of observed
    probes, in order to arrive at reliable abundances and abundance limits
    (the HI data are described in Paper II, Wakker et al.,
    2001ApJS..136..537W). Distances to stellar probes are revisited and
    calculated consistently, in order to derive distance brackets or
    limits for many of the clouds, taking care to properly interpret
    nondetections.

File Summary:
--------------------------------------------------------------------------------
 FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe            80        .   This file
table2a.dat      134      251   Published results for all HV/IV clouds
table2b.dat      203     1078   Published results for all probes of each
                                 HVC/IVC, sorted by cloud
cloud.dat         29       57   Cloud types
telescop.dat      65       22   Telescope names
refs.dat         264      129   References
notes.dat         80      278   Notes
--------------------------------------------------------------------------------

See also:
   J/ApJS/79/77 : Bell Lab. H I Survey - High Velocity Clouds (Stark+ 1992)

Byte-by-byte Description of file: table2a.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  2  I2    ---     CNum      Cloud number in cloud.dat file
   4- 19  A16   ---     Name      Cloud name
      21  A1    ---   l_Distu     Limit flag on Distu
  22- 26  F5.2  kpc     Distu     ? Distance to cloud or upper limit if
                                     Distl given
      28  A1    ---   l_Distl     Limit flag on Distl
  29- 33  F5.2  kpc     Distl     ? Lower limit on cloud distance
      35  A1    ---   l_Zupper    Limit flag on Zupper
  36- 40  F5.2  kpc     Zupper    ? Upper limit on cloud height above
                                     galactic plane
      42  A1    ---   l_Zlower    Limit flag on Zlower
  43- 47  F5.2  kpc     Zlower    ? Lower limit on cloud height above
                                     galactic plane
  49- 54  A6    ---     Ion       Ion name
  56- 67  E12.2 cm-2    Nion      ? Expected column density
      69  A1    ---   l_Abd       Limit flag on Abd
  70- 82  E13.2 ---     Abd       ? Ion abundance (Nion/NHI)
  84- 96  E13.2 ---   e_Abd       ? Uncertainty in Abd
  98-110  E13.2 ---     EAbd      ? Expected ion abundance
     112  A1    ---   l_DAbd      Limit flag on DAbd
 115-123  F9.6  Sun     DAbd      ? Derived abundance relative to solar
 125-134  A10   ---   n_Name      Notes on Name, comma-separated
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table2b.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label   Explanations
--------------------------------------------------------------------------------
   1-  2  I2    ---     CNum    Cloud number in cloud.dat file
       4  A1    ---   f_Name    [m] Indicates a mistaken claim of absorption
   6- 18  A13   ---     Name    Probe name
  20- 25  F6.2  deg     GLON    Galactic longitude
  27- 32  F6.2  deg     GLAT    Galactic latitude
  35- 39  F5.2  kpc     Dis     ? Probe distance
  42- 45  F4.2  kpc   e_Dis     ? Error in Dis
      47  A1    ---   f_Dis     Method of determination of Dis (2)
  50- 54  F5.2  kpc     Zheight ? Probe height above galactic plane
  56- 63  A8    ---     Type    Spectral type of star or classification of
                                  extra-galactic object
  65- 71  A7    ---     Cloud   Name of HV or IV cloud or complex
      73  A1    ---   f_vHVC    [abcu] Flag on vHVC (3)
  75- 78  I4    km/s    vHVC    ? LSR velocity of HVC or IVC toward probe
      80  A1    ---   l_NHI     Limit flag for NHI
  81- 90  E10.2 cm-2    NHI     ? HI column density of HVC/IVC
  92- 99  E8.2  cm-2  e_NHI     ? Error in NHI
 101-102  A2    ---     Tel     Telescope used to measure NHI in
                                 telescop.dat file
     104  A1    ---   f_Ion     [(] Indicates Ion data is superseded by
                                 newer measurements
 105-110  A6    ---     Ion     Observed ion
 112-115  I4    km/s    vION    ? LSR velocity of absorption
     117  A1    ---   l_Nion    Limit flag for Nion
 119-130  E12.2 cm-2    Nion    Column density for ion
                                  (see Note 5 when f_Nion = t)
 132-143  E12.2 cm-2  e_Nion    ? Error in Nion
     145  A1    ---   f_Nion    Note on determination of Nion (5)
     147  A1    ---   l_Abd     Limit flag for Abd
 148-160  E13.2 ---     Abd     ? Ion abundance (Nion/NHI)
 162-174  E13.2 ---   e_Abd     ? Error in Abd
     176  A1    ---   l_Asol    Limit flag Asol
 177-187  F11.6 ---     Asol    ? Ion abundance relative to solar abundance
                                  (see Note 5 when f_Nion = t)
     189  A1    ---     Drelev  Flag indicating whether probe gives relevant
                                 distance information (6)
 191-193  A3    ---   r_Name    Reference number in refs.dat file
     194  A1    ---     ---     [)] Closes off the column labelled f_Ion
 196-204  A9    ---   n_Name    Notes in notes.dat file, comma-separated
--------------------------------------------------------------------------------
Note (2): Method of determination of Distance:
     p = 1/parallax, as measured by Hipparcos;
     a = from detailed atmospheric analysis;
     g = use the distance of a globular cluster or the LMC;
     s = spectroscopic distance based on spectral type;
     t = spectroscopic distance based on spectral type, even though
          parallax was measured;
     r = value quoted in reference;
     E = extra-galactic object.
Note (3): Note on HVC velocity
     u = HVC velocity at which an upper limit to the HI column density is set;
     a = indicates the second component of a multicomponent absorption;
     b = indicates the second component of a multicomponent absorption;
     c = indicates the third component of a multicomponent absorption.
Note (5): Note on Column density for ion:
     N = Proper derivation done in reference;
     L = Log of column density given in reference;
     W = Converted from equivalent width;
     E = Detection inferred from large equivalent width;
     t = indicates a 21-cm observation. Nion column contains the column
          density of the absorbing cool HI and Abd column contains the
          optical depth of the absorption.
     S = Upper limit based on S/N ratio in spectrum.
Note (6): See Appendix A for further details.
     U = Detection in stellar spectrum sets upper limit
     l = Significant non-detection sets lower limit (limit on colum
          density below (expected value)/(safety factor))
     L = Significant non-detection sets lower limit (limit on column
          density below (expected value)/(3 times safety factor))
--------------------------------------------------------------------------------

Byte-by-byte Description of file: cloud.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  2  I2    ---     CNum      Cloud number
       4  A1    ---     ---       [=]
   6- 29  A24   ---     Type      Nature of the cloud
--------------------------------------------------------------------------------

Byte-by-byte Description of file: telescop.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  2  A2    ---     Tel       Telescope code
       4  A1    ---     ---       [=]
   6- 65  A60   ---     Text      Telescope
--------------------------------------------------------------------------------

Byte-by-byte Description of file: refs.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  3  I3    ---     Ref       Reference number
   5- 44  A40   ---     BibCodes  List of (up to 2) bibCode designating the
                                   articles
  46- 84  A39   ---     Aut       Author's name
  86-285  A200  ---     Com       Comments
--------------------------------------------------------------------------------

Byte-by-byte Description of file: notes.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  3  A3    ---     Note      Note code
   5- 80  A76   ---     Text      Text of the note
--------------------------------------------------------------------------------

History:
    From electronic version of the journal

References:
    Wakker et al., Paper II           2001ApJS..136..537W
================================================================================
(End)                    Greg Schwarz [AAS], Patricia Bauer [CDS]    14-Jan-2002

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