ACDS V10.0 - Detailed Description of VII/145

ACDS V10.0 - Fri May 03 05:54:56 CEST 2019

| # Detailed Description of VII/145 : Nearby Galaxies Catalogue (NBG) (Tully 1988) |

Note : this is the description file of the original catalog. This HTML page corresponds well to the original description, but some minor changes in the format may have been introduced in the FITS output files in order to allow for arithmetic operations on quantities such as coordinates and times. h:m:s and d:m:s units are normally converted into degrees, and YYYY-MM-DD into julian days.
Similarly, some slight changes may have been introduced in the units; the value given in the HTML files supersedes the value indicated in the ReadMe file for this catalogue.

    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

    ×                   80        .   This file
    × 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: this table contains all galaxies in "catalog", plus
         our Galaxy (the Milky Way)

    Byte-by-byte Description of file:  catalog.dat

       Bytes Format  Units   Label    Explanations

       1-  4  I4     ---     NBG      [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 (= 1/R25)
      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    RVel     Heliocentric velocity
      72- 74  I3     km/s    e_RVel   Mean error on RVel
          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  [solLum] 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 (=1/R25)
            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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               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.
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       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.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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    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