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1989CamPress.....Tully+

VII/145         Nearby Galaxies Catalogue  (NBG)     (Tully 1988)
=============================================================================
Nearby Galaxies Catalogue
      TULLY R.B
     
=============================================================================
ADC_Keywords: Galaxy catalogs ;

In CATS  there are no files groups, clusters
********************************************

Description (Introduction of Catalog):

This compendium is a companion to the Nearby Galaxies Atlas (ref. 29; hereafter NBG Atlas). Data has been accumulated on 2367 galaxies with systemic velocities less than 3000 kilometers/second. Any galaxy was admitted to the catalog if it had a known velocity in 1978 that satisfied the specified limit of 3000 kilometers/second, or if it was subsequently observed to have a suitable velocity in surveys of the entire sky by the author and collaborators (ref. 6, 11, 22).

There are many sources of velocities, so this catalog could potentially be quite heterogeneous. However, two sources dominate. One of these is the magnitude-limited Shapley-Ames sample, which assures the inclusion of all galaxies brighter than 12th magnitude in the blue passband (ref. 25). There are 1053 Shapley-Ames galaxies within the velocity limit. The other source was already mentioned: the all-sky survey in the neutral hydrogen line by the author and collaborators. This survey was undertaken after a complete reinspection of photographic atlases of the sky. This survey was insensitive to gas-deficient systems and has severe incompletion problems at velocities beyond 2000 kilometers/second (discussed in ref. 11). However, the virtue of our survey is homogeneous coverage across the unobscured part of the sky. The neutral hydrogen survey provides 1515 velocities to the catalog. There is some overlap between the two principal sources. It is this cumulative sample that is mapped in the NBG Atlas.

There are three parts to the catalog. The first and by far the largest section (catalog) provides information about each of the 2367 galaxies. One element of that information is a group affiliation, and in a second section (groups) there is a reordered listing that clarifies the composition of each group. The final, very short section (clusters) identifies the rich clusters of galaxies that delineate the supercluster complexes mapped in the last two plates of the NBG Atlas.

The text of the atlas is written at a level that can be appreciated by a wide audience. The material in this catalog and the following description are of a more technical nature. This catalog is intended for an audience of professional and motivated amateur astronomers.


File Summary:
----------------------------------------------------------------------------
  FileName      Lrecl  Records   Explanations
----------------------------------------------------------------------------
ReadMe             80        .   This file
catalog           328     2367   The Nearby Galaxies Catalog (NBG)
groups             48     2368  *Lists by groups
clusters           49      382   Identification of Rich clusters
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Note on groups: this table contains all galaxies in "catalog", plus
     our Galaxy (the Milky Way)
----------------------------------------------------------------------------

Byte-by-byte Description of file: catalog
----------------------------------------------------------------------------
   Bytes Format  Units   Label    Explanations
----------------------------------------------------------------------------
   1-  4  I4     ---     Seq      [1/2367]+ Running number
   6- 13  A8     ---     Name     Galaxy Name (1)
  15- 16  I2     h       RAh      Right Ascension 1950 (hours)
  17- 20  F4.1   min     RAm      Right Ascension 1950 (minutes)
      22  A1     ---     DE-      Declination 1950 (sign)
  23- 24  I2     deg     DEd      Declination 1950 (degrees)
  25- 26  I2     arcmin  DEm      Declination 1950 (minutes)
  28- 29  I2     ---     HubCode  [-5/13] Morphological type code (2)
  30- 31  A2     ---     HubPec   [BAXP ] Morphological peculiarities (2)
  34- 38  F5.1   arcmin  D25      ?=0 Observed diameter at 25mag/arcsec2
                                    isophote in blue (3)
  40- 44  F5.1   arcmin  D25bi    ?=0 Corrected diameter (4)
      46  A1     ---     r_D25bi  [926451] Reference for D25bi (5)
  48- 51  F4.2   ---     d/D      ]0/1]?=0. Axial ratio of minor to
                                    major diameter
  54- 56  F3.0   deg     i        inclination from face-on (6)
  58- 62  F5.2   mag     BTbi     ?=0. Blue apparent magnitude adjusted
                                    for reddening (7)
      64  A1     ---     r_BTbi   [0127635] Source for blue magnitudes (8)
  66- 70  F5.0   km/s    RadVel   Heliocentric velocity
  72- 74  I3     km/s   e_RadVel  Mean error on RadVel
      76  I1     ---     RefHI    ]0/7]?=0 Reference to HI observation (9)
  78- 82  F5.0   km/s    V0       Systemic velocity (solar motion of 300km/s)
  85- 90  F6.2   deg     GLON     Galactic longitude
  92- 97  F6.2   deg     GLAT     Galactic latitude
  99-104  F6.2   deg     SGLON    Supergalactic longitude as in RC2
 106-111  F6.2   deg     SGLAT    Supergalactic latitude as in RC2
 113-118  F6.2   mag     MB       ?=0 Absolute blue magnitude of galaxy
 120-124  F5.2   mag     m-M      Distance modulus (5log(R)+25)
 126-129  F4.1   Mpc     R        Distance, assuming H=75km/s/Mpc (10)
 131-135  F5.1   kpc     Delta25  ?=0 Linear diameter (0.292 . D25bi * R)
 137-141  F5.1   Mpc     SGX      X coordinate in SuperGalactic frame
 143-147  F5.1   Mpc     SGY      Y coordinate in SuperGalactic frame
 149-153  F5.1   Mpc     SGZ      Z coordinate in SuperGalactic frame
 156-160  F5.2   mag     H-0.5bi  ?=0 Apparent magnitude at 1.6um
                                    adjusted for reddening (10)
 162-166  F5.2   mag     B-H      color (note: different apertures in B and H)
 168-171  F4.2   mag     ABi0     Obscuration within candidate galaxy (10)
 173-176  F4.2   mag     ABb      Obscuration within Milky Way
 179-181  I3     km/s    W20      ?=0 HI line width at 20% maximum (10)
 182-184  I3     km/s    e_W20    ?=0 Uncertainty on W20
 186-188  I3     ---     r_W20    [2/301]?=0 Source for W20 (11)
 190-193  F4.0   km/s    WR       ?=0 Rotational velocity profile width
                                    parameter (10)
 195-198  F4.0   km/s    WDi      ?=0 Global velocity, dynamical profile
                                    width parameter (10)
 201-205  F5.210+6solMass/Mpc2 logFc  ?=-9.99 log of HI flux
                                    adjusted for resolution effects
 206-208  I3     %       e_logFc  ]0/100]?=0 Relative error on logFc
 210-212  I3     ---     r_logFc  ?=0 Reference (source) for logFc (11)
 214-217  F4.2   ---     fH       ?=0 Flux correction factor (12)
 219-223  F5.2   solMass log(MH)  ?=0 mass of HI (10)
 225-229  F5.2   solMass log(MT)  ?=0 Total mass of Galaxy (10)
 231-235  F5.3   ---     MH/MT    ?=0 ratio of HI to total mass (16)
 237-241  F5.2   Sun     log(LB)  ?=0 Intrinsic blue luminosity of galaxy (10)
 243-246  F4.2   Sun     MH/LB    ?=0 ratio of HI to blue luminosity
 248-252  F5.2   Sun     MT/LB    ?=0 Mass to blue luminosity ratio
 255-258  F4.2   Mpc-3   rho      ?=0 Density of galaxies (13)
 260-267  A8     ---     Group    [ 0-9+-] Group affiliation (14)
 270-275  A6     ---     UGC/ESO  Designation in UGC (number <= 12921) or ESO
 277-285  A9     ---     MCG      designation in MCG (Ref. 35)
     287  A1     ---     inRC2    [2] '2' when the galaxy in RC2 (ref. 9)
 289-328  A40    ---  OtherNames  Other names separated by a comma (15)
----------------------------------------------------------------------------
Note (1): Entries are identified, in order of priority, by a
  NGC number (preceded by N), or by an UGC number (preceded by U),
  or by a name constructed from equatorial coordinates. See also
  other names in the four rightmost columns.
Note (2): the morphological type is given by a numeric code
        that is slightly different from RC2 one
        -5   E   Elliptical
        -3 E/SO  Elliptical/Lenticular (classification uncertain)
        -2  SO   Lenticular
         0  SO/a Lenticular/Spiral
         1  Sa   Spiral
         2  Sab  Spiral
         3  Sb   Spiral
         4  Sbc  Spiral
         5  Sc   Spiral
         6  Scd  Spiral
         7  Sd   Spiral
         8  Sdm  Spiral
         9  Sm   Spiral/irregular
        10  Ir   Irregular
        12  S    Spiral/irregular (classification uncertain)
        13  P    Peculiar
    Following the morphology number is a "B" (bar), "A" (absence of
    a bar), "X" (intermediate case), "P" (existence of a peculiarity)
Note (3): Conversions from diameters in the major catalogues are:
   log(D25) = 0.983(D(UGC) + 0.3) - 0.051
   log(D25) = 0.998(D(ESO) + 0.3) - 0.132
   log(D25) = 1.020(D(MCG) + 0.3) - 0.007
Note (4): Diameter adjusted for effects of projection and obscuration.
    Adjustments are made according to the equation
    log(D25bi) = log(D25) - c log(D/d) + ABb.KD25,  where
        D/d  is the ratio of major to minor diameter
        c    = 0.22
        ABb  is the Galactic (Milky Way) absorption in blue
        KD25 = 0.09
Note (5): Source of diameter in decreasing order of priority
    9 = standards (ref.12)
    2 = UGC (ref.20)
    6 = ESO (ref.16)
    4 = MCG (ref.35)
    5 = BCG (ref.7)
    1 ** unspecified
Note (6): The inclination is almost always given by
    i = 3deg + acos(sqrt(((d/D)^2 - 0.2^2)/(1 - 0.2^2)))
Note (7): BTbi is computed from:
    BTbi = BT - ABb - ABi0
Note (8): Source of blue magnitudes in decreasing order of priority:
    1 = Holmberg (ref.14)
    2 = RC2 (ref.9)
    7 = deVaucouleurs (ref.8)
    6 = miscellaneous
    3 = CGCG (ref.36)
    5 = Harvard (ref.7)
Note (9): The telescopes used are NRAO 91m and 43m,
    the Max-Planck-Institut 100m and Parkes 64m, according
    to the following code:
    Code Telescope  Resolution
      1        91      22 km/s
      2        43      22
      3        91       5.5
      4        43       5.5
      5       100       5.5
      6       100      22
      7        64       4.9
Note (10): See also notes in the printed catalogue
Note (11): Hydrogen line width and Flux literature references
    2 R.J. Allen, B.F. Darchy, and R. Lauque, A&A 10,198, 1971.
    3 R.J. Allen, W.M. Goss, R. Sancisi, W.T. Sullivan, III, and
           H. van Woerden. In "The Formahon and Dynamics of Galaxies",
           IAU Symposium, no. 58, ed. J.R. Shakeshaft, p.425.
           Dordrecht: Reidel, 1974.
    5 C. Balkowski, L. Bottinelli, P. Chamaraux, L. Gouguenheim, and
           J. Heidmann, A&A 34, 43, 1974.
    6 C. Balkowski, L. Bottinelli, L. Gouguenheim, and J. Heidmann,
           A&A 21, 303, 1972.
    7 C. Balkowski, L. Bottinelli, L. Gouguenheim, and J. Heidmann,
           A&A 23, 139, 1973.
   10 L. Bottinelli, P. Chamaraux, L. Gouguenheim, and J. Heidmann,
           A&A 29, 217, 1973.
   11 L. Bottinelli, P. Chamaraux, L. Gouguenheim, and R. Lauque,
           A&A 6, 453, 1970.
   12 L. Bottinelli, R. Duflot, L. Gouguenheim, and J. Heidmann,
           A&A 41, 61, 1975.
   17 L. Bottinelli, L. Gouguenheim, and J. Heidmann, A&A 22, 281, 1973.
   20 N. Carozzi, P. Chamaraux, and R. Duflot-Augarde, A&A 30, 21, 1974.
   21 P. Chamaraux, J. Heidmann, and R. LauqueLA, A&A 8, 424, 1970.
   24 R.D. Davies, and B.M. Lewis, MNRAS 165, 231, 1973.
   25 J. E Dean, and R. D. Davies, MNRAS 170, 503, 1975.
   36 L. Gouguenheim, A&A 3, 281, 1969.
   41 W. Huchtmeier, A&A 17, 207, 1972.
   51 B.M. Lewis, and R.D. Davies, MNRAS 165, 213, 1973.
   54 W.H. McCutcheon, and R.D. Davies, MNRAS 150, 337, 1970.
   56 S.D. Peterson, and G.S. Shostak, AJ 79, 767, 1974.
   60 M.S. Roberts, AJ, 73, 945, 1968.
   66 B.J. Robinson, and K.J. van Damme, Australian J. Physics, 19, 111, 1966.
   67 B.J. Robinson, and J.A. Koehler, Nature, 208, 993, 1965.
   69 D.H. Rogstad, I.A. Lockhard, and M.C.H. Wright, ApJ 193, 309, 1974.
   72 D.H. Rogstad, and G.S. Shostak, A&A 22, 111, 1973.
   76 R.R. Sholbrook, and B.J. Robinson, Australian J. Physics, 20, 131, 1967.
   77 G.S. Shostak, ApJ 187, 19, 1974.
   79 G.S. Shostak, ApJ 198, 527, 1975.
   80 G.S. Shostak, and D.H. Rogstad, A&A 24, 405, 411, 1973.
   96 E.E. Epstein, AJ 69, 490, 1964.
  102 J.V. Hindman, F.J. Kerr, and R.X. McGee, Australian J. Physics,
            16, 570, 1963.
  105 L. Volders, and J.A. Hogbom, Bull. Astron. Inst. NL, 15, 307, 1961.
  106 J. Heidmann, Bull. Astron. Inst. NL, 15, 314, 1961.
  201 W.K. Huchtmeier, G.A. Tammann, and H.J. Wendker, A&A 46, 381, 1976.
  202 W.K. Huchtmeier, G.A. Tammann, and H.J. Wendker, A&A 57, 313, 1977.
  203 B. Balick, S.M. Faber, and J.S. Gallagher, ApJ 209, 710, 1976.
  204 J.S. Gallagher, S.M. Faber, and B. Balick, ApJ 202, 7, 1976.
  205 G.R. Knapp, J.S. Gallagher, S.M. Faber, and B. Balick, ApJ 82, 106, 1977.
  206 A. Bosma, R.D. Ekers, J. Lequeux, A&A 57, 97, 1977.
  208 D.A. Cesarsky, E.G. Falgarone, and J. Lequeux, A&A 59, L5, 1977.
  209 P. Chamaraux, A&A 60, 67, 1977.
  210 J.H. Bieging, and P. Biermann, A&A 6b, 361, 1977.
  211 J.R. Dickel, and H.J. Rood, ApJ 223, 391, 1978.
  212 R.J. Allen, J.M. van der Hulst, W.M. Goss, and W. Huchtmeier,
          A&A 64, 359, 1978.
  214 C. Balkowski, P. Chamaraux, and L. Weliachew, A&A 69, 263, 1978.
  216 J.H. Bieging, A&A 64, 23, 1978.
  217 G.S. Shostak, A&A 68, 321, 1978.
  218 T.D. Kinman, V.C. Rubin, N. Thonnard, W.K. Ford, Jr., and
            C.J. Peterson, ApJ 82, 871, 1977.
  220 G.D. van Albada, A&A 61, 297, 1977.
  222 A.J. Longmore, T.G. Hawarden, B.L. Webster, W.M. Goss, and
            U. Mebold, MNRAS 184, 97P, 1978.
  223 N. Krumm, and E.E. Salpeter, ApJ 227, 776, 1979.
  225 K.Y. Lo, and W.L.W. Sargent, ApJ 227, 756, 1979.
  226 T.X. Thuan, and P.D. Seitzer, ApJ 231, 327, 1979.
  300 G. Helou, C. Giovanardi, E.E. Salpeter, and N. Krumm, ApJS 46, 267, 1981.
  301 K. Reif, U. Mebold, W.M. Goss, H. van Woerden, and B. Siegman,
          A&AS 50, 451, 1982.
Note (12): All HI observations by the author and collaborators were
    single-beam measurements with a beam that is frequently smaller
    than the size of the source. The corrections are discussed in Ref.11
Note (13): density of galaxies brighter than -16mag in the vicinity
    of the entry. The local density was determined on a 3D-grid at
    0.5Mpc spacing. See the details in the printed catalogue
Note (14): galaxies may be affiliated with other galaxies in groups,
    associations, or clouds. The affiliations are described by a code
    in the form  AB+/-CD+EF :
    a galaxy is located in cloud AB (see Note (1) in table "groups"),
    group -CD  or first level association +CD,
    and second level association +EF.
    Galaxies are ordered by group in table "groups"
Note (15): The alternative names are that date back before 1976 can be
    found in BGC (ref.7) and RC2 (ref.9). More recent sources are designated
      Arak   = Arakelian       (ref. 3)
      CVndw  = Lo and Sargent  (ref.18)
      Kar    = Karachentseva   (ref.15)
      M81dw  = Lo and Sargent  (ref.18)
      RMB    = Rubin et al.    (ref.24)
      SAGDIG = Cesarsky et al. (ref. 5)
      SCLDIG = Laustsen et al. (ref.17)
      Scl    = Rubin et al.    (ref.23)
      Turn   = Turner          (ref.32)
      UGCA   = Nilson          (ref.21)
      UKS    = Longmore et al. (ref.19)
    At the very end of this column there may be a notation that indicates
    if the galaxy has a Seyfert(S) or LINER(L) active nucleus;
    the number that follows specifies whether the type is 1, or 2,
    or an intermediate case.
Note (16): is sometimes larger than 1 due to the different methods
    for the computations of MH and MT
----------------------------------------------------------------------------
Byte-by-byte Description of file: groups
----------------------------------------------------------------------------
   Bytes Format  Units   Label    Explanations
----------------------------------------------------------------------------
   1-  8  A8     ---     Group    [ 0-9+-] Group identification (1)
  13- 20  A8     ---     Name     Galaxy name, as in catalog
  24- 25  I2     ---     HubCode  [-5/13] Morphological type code
  26- 27  A2     ---     HubBar   [BAXP ]
  31- 36  F6.2   mag     MB       ? Absolute blue magnitude of galaxy
      37  A1     ---     MWay     [*] flag for our Galaxy
  41- 45  F5.0   km/s    V0       Systemic velocity
----------------------------------------------------------------------------

Note (1): the first two digits designate the Cloud, as follows:
    11=Virgo Cluster and Southern Extension
    12=Ursa Major Cloud
    13=Ursa Major Southern Spur
    14=Coma - Sculptor Cloud
    15=Leo Spur
    16=Centaurus Spur
    17=Triangulum Spur
    18=Perseus Cloud
    19=Pavo - Ara Cloud
    21=Leo Cloud
    22=Crater Cloud
    23=Centaurus Cloud
    24=Lynx Cloud
    31=Antlia - Hydra Cloud
    32=Cancer - Leo Cloud
    33=Carina Cloud
    34=Lepus Cloud
    41=Virgo - Libra Cloud
    42=Canes Venatici - Camelopardalis Cloud
    43=Canes Venatici Spur
    44=Draco Cloud
    45=Coma Cloud
    51=Fornax Cluster and Eridanus Cloud
    52=Cetus - Aries Cloud
    53=Dorado Cloud
    54=Antlia Cloud
    55=Apus Cloud
    61=Telescopium - Grus Cloud
    62=Pavo - Indus Spur
    63=Pisces - Austrinus Spur
    64=Pegasus Cloud
    65=Pegasus Spur
    66=Sagittarius Cloud
    71=Serpens Cloud
    72=Bootes Cloud
    73=Ophiuchus Cloud
    Other (multiple of 10) are Isolated groups.
----------------------------------------------------------------------------

Byte-by-byte Description of file: clusters
----------------------------------------------------------------------------

   Bytes Format  Units   Label    Explanations
----------------------------------------------------------------------------

   1-  3  A3     ---     SuperCl  Complex/Supercluster designation (1)
       5  A1     ---     Flag     [+*] See Note (2)
   7- 17  A11    ---     Cluster  designation (Abell or Anonymous)
  21- 26  F6.4   ---     z        Redshift
  31- 35  F5.0   Mpc     SGX      X coordinate in SuperGalactic frame
  38- 42  F5.0   Mpc     SGY      Y coordinate in SuperGalactic frame
  45- 49  F5.0   Mpc     SGZ      Z coordinate in SuperGalactic frame
----------------------------------------------------------------------------

Note (1): the notation is A.B, where A designates a complex, and A.B
       the Supercluster, as follows:
    1   PISCES - CETUS SUPERCLUSTER COMPLEX
    1.1    Pisces - Cetus Supercluster
    1.2    Perseus - Pegasus Chain
    1.3    Pegasus - Pisces Chain
    1.4    Sculptor Region
    1.5    Virgo - Hydra - Centaurus Supercluster
    2   AQUARIUS SUPERCLUSTER COMPLEX
    2.1    Aquarius - Capricornus Region
    2.2    Aquarius Region
    3   HERCULES - CORONA BOREALIS SUPERCLUSTER COMPLEX
    3.1    Hercules Supercluster
    3.2    Bootes Supercluster
    3.3    Corona Borealis Supercluster
    3.4    Corona Borealis - Hercules Supercluster
    4   LEO SUPERCLUSTER COMPLEX
    4.1    Leo Supercluster
    4.2    Leo - Coma Supercluster
    4.3    Sextans Supercluster
    5   URSA MAJOR SUPERCLUSTER COMPLEX
    5.1    Ursa Major Supercluster
    5.2    Draco Supercluster
Note (2): the '*' indicates the cluster is in a sufficiently dense region
    in the core of the complex that a pathway can be found to every other
    cluster with an '*' in the same complex with cluster-to-cluster steps
    of less than 40Mpc.
    The '+' designates associations with the incompletely surveyed
    Indus region.
----------------------------------------------------------------------------

References:
   1. Aaronson, M., J. Huchra, J.R. Mould, R.B. Tully, J.R. Fisher,
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      H. van Woerden, unpublished.
   7. de Vaucouleurs, G., and A. de Vaucouleurs. Reference Catalogue of
      Bright Galaxies. Austin: University of Texas Press, 1964 (BGC).
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      AJ 86, 1429, 1981.
   9. de Vaucouleurs, G., A. de Vaucouleurs, and H.G. Corwin, Jr. Second
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      Press, 1976 (RC2).
  10. Dreyer, J.L.E. New General Catalogue of Nebulae and Clusters of
      Stars, 1888. Reprinted in Mem. R. Astron. Soc., 1962 (NGC).
  11. Fisher, J.R., and R.B. Tully. ApJS 47, 139, 1981.
  12. Fouque, P., and G. Paturel. A&AS 53, 351, 1983.
  13. Fouque, P., and G. Paturel. A&A 150, 192, 1985.
  14. Holmberg, E.B., Meddelande Lunds Obs., Series II, No. 136, 1958.
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      Munchen (Germany): European Southern Observatory, 1982 (ESO).
  17. Laustsen, S., W. Richter, J. van der Lans, R.M. West, and
      R.N. Wilson. A&A 54, 639, 1977.
  18. Lo, K.Y., and W.L.W. Sargent, ApJ 227, 756, 1979.
  19. Longmore, A.J., T.G. Hawarden, B.L. Webster, W.M. Goss, and
      U. Mebold, MNRAS 184, 97P, 1978.
  20. Nilson, P., Uppsala General Catalogue of Galaxies. Uppsala, Sweden:
      Societatis Scientiarum Upsaliensis, 1973 (UGC).
  21. Nilson, P., Catalogue of Selected Non-UGC Galaxies, Uppsala
      Astron. Obs. Rep. No. 5, 1974.
  22. Reif, K., U. Mebold, W.M. Goss, H. van Woerden, and B. Siegman,
      A&A 50, 451, 1982.
  23. Rubin, V.C., W.K. Ford, Jr., N. Thonnard, M.S. Roberts, and
      J.A. Graham, AJ 81, 687, 1976.
  24. Rubin, V.C., S. Moore, and E.C. Bertiau, AJ 72, 59, 1967.
  25. Sandage, A., AJ 83, 711, 1978.
  26. Tully, R.B., ApJ 321, 280, 1987.
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  28. Tully, R.B. AJ 96, 73, 1988.
  29. Tully, R.B., and J.R. Fisher. Nearby Galaxies Atlas. Cambridge:
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  36. Zwicky, E,E. Herzog, P. Wild, M. Karpowicz, and C.T. Kowal,
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      Pasadena: California Institute of Technology, 1961-68 (CGCG).

Historical Notes:
  * The original files were received from ADC/Greenbelt in 1994
    as 3 data files tully.data1, tully.data2 and tully.data3,
    and a Fortran program tully.software to read the parameters of
    a galaxy which are on three lines in the file tully.data3
  * 04-Jul-1995: data files converted to standard tables.
    A control character \001 in record#2168 (2119-45)
    has been removed, and the ReadMe file was generated.
================================================================================
(End)                                    Francois Ochsenbein [CDS]   20-Jul-1994

CDS Catalogue Service