VII/151     Structure Parameters of Galactic Globular Clusters (Webbink 1985)

Structure Parameters of galactic Globular Clusters Webbink, R.F. <IAU Symp 113 "Dynamics of Star Clusters", Ed. J. Goedman & P. Hut, 541 (1985)>
ADC_Keywords: Clusters, globular ; Magnitudes Description: This catalog contains observed and derived structure parameters for 154 galactic globular clusters, 7 dwarf spheroidal satellites of the Galaxy, and 6 globular clusters in the Fornax dwarf spheroids, respectively, in six different files. Files 1-3 (table1a, table1b, & table1c) list observed parameters, including cluster designation in order of right ascension, equatorial coordinates (B1950), apparent level of the cluster horizontal branch, reddening, subgiant branch color, limiting and core angular radii, ellipticities (only for table1b), integrated magnitude and central surface brightness. Files 4-6 (table2a, table2b, & table2c) contain positional and structural data derived from the observational data of table1. These include, for instance, galactic and galactocentric or Cartesian coordinates, heliocentric and galactocentric distances, or angular and projected linear distances, position angle, metallicity, limiting and core radii, central relaxation time scale, central mass density, central velocity dispersion, and central escape velocity. The references (all columns which label start by r_) are not available in electronic form. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1a.dat 172 154 Observed Galactic Clusters table1b.dat 172 7 Observed Galactic Dwarf Spheroidals table1c.dat 172 6 Observed Fornax Globular Clusters table2a.dat 155 154 Derived Galactic Clusters table2b.dat 155 7 Derived Galactic Dwarf Spheroidals table2c.dat 155 6 Derived Fornax Globular Clusters -------------------------------------------------------------------------------- See also: VII/13 : Globular Cluster Catalogue (Arp 1965) VII/103 : Catalogue of Galactic Globular Clusters (Monella, 1985) Byte-per-byte Description of file: table1a.dat table1b.dat table1c.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- IAU Cluster designation 11- 23 A13 --- Name1 Cluster name 25- 32 A8 --- Name2 Cluster name 35- 36 I2 h RAh Right ascension 1950 38- 39 I2 min RAm Right ascension 1950 41- 42 I2 s RAs Right ascension 1950 45 A1 --- DE- Declination 1950 sign 46- 47 I2 deg DEd Declination 1950 49- 52 F4.1 arcmin DEm Declination 1950 55- 59 F5.2 mag VHB ? Apparent level of the cluster horizontal branch 60 A1 --- u_VHB Uncertainty flag (:) on VHB 62- 63 A2 --- m_VHB Method used for the determination of VHB (1) 66- 68 A3 --- r_VHB Reference of VHB determination 70 A1 --- l_EBV [>] Limit flag for EBV 71- 75 F5.3 mag EBV Color excess E(B-V) 76 A1 --- u_EBV Uncertainty flag (:) on EBV 77- 79 A3 --- m_EBV Method used for the determination of EBV (2) 81- 83 A3 --- r_EBV Reference for EBV determination 85- 88 F4.2 mag BVg ?observed color of the cluster subgiant branch 89 A1 --- u_BVg Uncertainty flag (:) on BVg 92- 93 A2 --- m_BVg Method for the determination of BVg (3) 96- 98 A3 --- r_BVg Reference for BVg determination 101-106 F6.3 arcmin lgtt ?log(radius) expressed in arcmin 107-108 A2 --- u_lgtt [: ] Uncertainty flag (:) on lgtt 109-110 A2 --- m_lgtt Method for the determination of lgtt (4) 114-116 A3 --- r_lgtt Reference for lgtt determination 119-123 F5.2 arcmin lgtc ?log(core radius) expressed in arcmin 124 A1 --- u_lgtc Uncertainty flag (:) on lgtc 126-127 A2 --- m_lgtc Method for the determination of lgtc (4) 130-132 A3 --- r_lgtc Reference for lgtc determination 134-137 F4.2 --- eps ]0/1]? Ellipticity (5) 139-143 F5.2 mag Vt ?Integrated V magnitude 144 A1 --- u_Vt Uncertainty flag (: or )) on Vt 146-148 A3 --- m_Vt Method for the determination of Vt (6) 150-152 A3 --- r_Vt Reference for Vt determination 156 A1 --- l_Sc [<] Limit flag for Sc 157-161 F5.2 mag/arcmin2 Sc ? Central surface brightness 162 A1 --- u_Sc [:)] Uncertainty flag (: or )) on Sc 165-167 A3 --- m_Sc Method for the determination of Vt and Sc (6) 170-172 A3 --- r_Sc Reference for the determination of Vt and Sc -------------------------------------------------------------------------------- Note (1): the method is coded as follows: CM = color-magnitude diagram (± 0.05) RR = mean magnitudes of RR Lyr variable (± 0.1) BG = magnitudes of the brightest giants (± 0.3) IR = combination of the index of richness, integrated apparent magnitude, estimated foreground reddening (± 0.6) A = foreground reddening plus assumed reddening law (± 1.4) Note (2): the method is coded as follows: HB = two-color diagram of blue horizontal branch (HB) stars NB = narrow-band photometry and spectroscopy of HB stars fit to model atmospheres B = color-magnitude diagram of blue HB stars fit to a fiducial curve rr = Sturch's method using RR Lyr colors at minimum RR = mean RR Lyr colors psi = slope of red continuum of individual giants DU = correlation of UV excesses of giant stars UB = asymptotic reddening of foreground stars in UBV uy = asymptotic reddening of foreground stars in uvby XY = asymptotic reddening of foreground stars in Vilnius photometry GB = blue edge of RR Lyr gap RD = red edge of RR Lyr gap CS = integrated optical or near-UV colors IR = integrated IR colors MI = correlation of metallicity index with integrated color HI = neutral Hydrogen column density plus galaxy counts CX = modified cosecant law Note (3): the method is coded as follows: CM = color-magnitude diagram DP = period difference of RR Lyr variables DS = cluster metallicity in individual RR Lyr UB = integrated UBV colors Q = line blanketing index from integrated narrow-band photometry BV = integrated BV colors Note (4): the method is coded as follows: SC = star counts SP = surface photometry AP = concentric aperture photometry D = correlation of apparent diameter with limiting radius e = eye estimate of the corde radius Note (5): the ellipticity only exists for table1b; methods and references for its determination are identical to the radius determinations lgtt and lgtc Note (6): the method is coded as follows: AP = concentric aperture photometry SP = surface photometry Sig = summation R = fit of the upper end of LF IR = index of richness -------------------------------------------------------------------------------- Byte-per-byte Description of file: table2a.dat table2b.dat table2c.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- IAU Cluster designation 11- 23 A13 --- Name1 Cluster name 25- 32 A8 --- Name2 Cluster name 35- 41 F7.3 deg GLON Galactic longitude 45- 51 F7.3 deg GLAT Galactic latitude 55- 59 F5.1 kpc Rdist ?Heliocentric distance 61- 66 F6.1 kpc Xdist ?Galactocentric distance 68- 73 F6.1 kpc Ydist ?Galactocentric distance 75- 80 F6.1 kpc Zdist ?Galactocentric distance 81- 86 F6.1 kpc rGC ?Galactocentric distance 88 A1 --- l_[m/H] Limit on [m/H] 89- 93 F5.2 Sun [m/H] ?log(metallicity) relative to Sun 96-101 F6.2 mag Mv ?Integrated absolute magnitude of the cluster 103 A1 --- l_rc [<] Limit flag on rc 104-109 F6.2 pc rc ?Core radius 113-118 F6.1 pc rt ?Limiting radius 121-125 F5.2 --- c ? Core Concentration parameter = log(rt/rc) 127 A1 --- l_lg.tr [<] Limit flag on lg.tr 128-133 F6.3 yr lg.tr ?log of central relaxation time (yr) 136 A1 --- l_lg.rho Limit flag on lg.rho 137-142 F6.3 solMass/pc3 lg.rho ?log of central mass density (solar masses per cubic parsec) 144 A1 --- l_s0 Limit flag on s0 145-149 F5.2 km/s s0 ?Central velocity dispersion 150 A1 --- l_Vesc Limit flag on Vesc 151-155 F5.1 km/s Vesc ?Central escape velocity -------------------------------------------------------------------------------- Historical Notes: * 12-Jan-1993: The catalogue was prepared at CDS (M.J. Wagner) from the printed catalogue. * 22-Aug-1996: Documentation and files converted to CDS Standards
(End) Francois Ochsenbein [CDS] 22-Aug-1996
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line