J/AJ/124/782       Bar galaxies and their environments    (van den Bergh+, 2002)

Bar galaxies and their environments. van den Bergh S. <Astron. J. 124, 782 (2002)> =2002AJ....124..782V 2002AJ....124..782V
ADC_Keywords: Clusters, galaxy ; Morphology Keywords: galaxies: clusters: general - galaxies: spiral Abstract: The prints of the Palomar Sky Survey, luminosity classifications, and radial velocities were used to assign all northern Shapley-Ames galaxies to either (1) field, (2) group, or (3) cluster environments. This information for 930 galaxies shows no evidence for a dependence of bar frequency on galaxy environment. This suggests that the formation of a bar in a disk galaxy is mainly determined by the properties of the parent galaxy, rather than by the characteristics of its environment. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 18 392 Northern Shapley-Ames Field Galaxies table2.dat 18 144 Northern Shapley-Ames Group Galaxies table3.dat 18 395 Northern Shapley-Ames Cluster Galaxies -------------------------------------------------------------------------------- See also: VII/51 : Revised Shapley-Ames Catalog of Bright Galaxies (Sandage+, 1981) J/A+AS/104/179 : Surface photometry in Shapley-Ames galaxies (Goudfrooij+ 1994) J/A+AS/114/21 : Shapley-Ames Galaxies at 2.8cm (Niklas+, 1995) Byte-by-byte Description of file: table1.dat table2.dat table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- Name Galaxy name 9- 14 A6 --- MType Morphological type 16- 18 A3 --- Pop Population (1) -------------------------------------------------------------------------------- Note (1): Population: S: cluster in which most galaxies are spirals E: cluster in which most galaxies are ellipticals E+S: cluster with a mixed population (spirals and ellipticals) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 12-Sep-2002
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