Astronomical Data Center
ADC/CDS Standard Document for Catalog:
/catalogs/7/7145/

The following is the "ReadMe" document that describes this ADC catalog. You can 
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ftp://adc.gsfc.nasa.gov/pub/adc/archives/catalogs/7/7145/. Or you can preview 
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VII/145         Nearby Galaxies Catalogue  (NBG)     (Tully 1988)
================================================================================
Nearby Galaxies Catalogue
      Tully R.B.
     <Cambridge University Press (1988)>
================================================================================
ADC_Keywords: Galaxy catalogs

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.dat    328       2367    The Nearby Galaxies Catalog (NBG)
groups.dat      48       2368   *Lists by groups
clusters.dat    49        382    Identification of Rich clusters
--------------------------------------------------------------------------------
Note on groups.dat: this table contains all galaxies in "catalog.dat", plus
     our Galaxy (the Milky Way)

Byte-by-byte Description of file: catalog.dat
--------------------------------------------------------------------------------
   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  F5.2   10+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
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    3 R.J. Allen, W.M. Goss, R. Sancisi, W.T. Sullivan, III, and
           H. van Woerden. In "The Formahon and Dynamics of Galaxies",
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    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.
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   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.
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  202 W.K. Huchtmeier, G.A. Tammann, and H.J. Wendker, A&A 57, 313, 1977.
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  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.
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            U. Mebold, MNRAS 184, 97P, 1978.
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  225 K.Y. Lo, and W.L.W. Sargent, ApJ 227, 756, 1979.
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  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.dat"
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.dat
--------------------------------------------------------------------------------
   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.dat
--------------------------------------------------------------------------------
   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.
--------------------------------------------------------------------------------

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  31. Tully, R.B., and E.J. Shaya. ApJ 281, 31, 1984.
  32. Turner, E.L., ApJ 208, 20, 1976.
  33. van den Bergh, S., ApJ 131, 215, 1960.
  34. van den Bergh, S., AJ 71, 922, 1966.
  35. Vorontsov-Velyaminov, B.A., A.A. Krasnogorskaya, and V.P. Arkipova.
      Morphological Cahlogue of Galaxies, Vols.  1-5. Moscow:
      Sternberg Institution, 1962-74 (MCG).
  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

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