VII/103 Galactic Globular Clusters (Monella 1985) ================================================================================ Catalogue of Galactic Globular Clusters Monella R. ================================================================================ ADC_Keywords: Clusters, globular Description: The catalogue collects, for the first time, the most important data concerning all the galactic globular clusters still well known. Here the objects enclosed in famous publications like the ones of Arp (1965), Alter et al. (1970), Alcaino (1973) are reported, with the addition of new clusters noticed recently (TER, ESO, UKS, TJ) and till KOD 1, found by K. Kodaira in July 1983 (IAUC 3846). The most important disposable data in literature have been found about every object. For the clusters found recently, the data may be fragmentary and susceptible of variations. A particular care has been utilized in the research of the most reliable informations and data, that have been homogenized and put in order later on. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 120 160 Data of Galactic Globular Clusters -------------------------------------------------------------------------------- See also: VII/151 : Structure Parameters of Galactic Globular Clusters (Webbink 1985) Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 4 I3 --- ID [1,160]+ Running number 7- 9 A3 --- Const Constellation of belonging 12- 21 A10 --- Name Common name of the globular cluster 24- 25 I2 h RAh Right Ascension 1950 (hours) 27- 28 I2 min RAm Right Ascension 1950 (minutes) 30- 31 I2 s RAs [0/60[? Right Ascension 1950 (seconds) 33 A1 --- DE- Declination 1950 (sign) 34- 35 I2 deg DEd Declination 1950 (degrees) 37- 40 F4.1 arcmin DEm Declination 1950 (minutes) 43- 47 F5.2 mag V ? Photovisual apparent integrated magnitude 49- 54 F6.2 mag Mv ? Photovisual absolute integrated magnitude 56- 60 A5 --- Sp Spectral integrated class 63- 67 F5.2 [Sun] [Fe/H] ? Degree of metallicity 70- 74 F5.2 arcmin appD ? Photographic apparent diameter 76- 80 F5.1 pc Diam ? Real diameter 84- 87 F4.1 mag m(BS) ? Apparent magnitude of the brightest star 89- 93 F5.1 kpc Gdist ? Distance from the center of our Galaxy 94- 95 A2 --- --- [00] 97-101 F5.1 kpc Sdist ? Distance from Sun 102-103 A2 --- --- [00] 105-108 A4 --- cClas Concentration class according to Sawyer-Hogg 110-113 I4 km/s RVel ? Radial velocity 115-117 I3 --- Nv ? Number of variables found in the cluster 118-120 A3 --- u_Nv [(?)] Uncertainty note -------------------------------------------------------------------------------- Historical note: The distance d of cluster#8 was corrected from 16.4 to 116.4kpc to agree with the publication. Author: R. MONELLA Sharru Astronomical Observatory, Via Giovanni XXIII, 13, 24050 COVO (Bergamo), Italy References: Arp, H. 1965, ApJ, 141, 43 (1965ApJ...141...43A) Alcaino, G. 1974, A&AS, 13, 55 (1974A&AS...13...55A) Alcaino, G. 1974, A&AS, 18, 9 (1974A&AS...18....9A) ================================================================================ (End) Francois Ochsenbein [CDS]; C.-H. Joseph Lyu [Hughes STX/NASA] 26-Sep-1996