V/19                Masses and Ages of Stars in 68 Open Clusters (Piskunov 1980)

Catalog of Masses and Ages of Stars in 68 Open Clusters Piskunov A. =1980BICDS..19...67P 1980BICDS..19...67P
ADC_Keywords: Clusters, open ; Stars, ages ; Stars, masses Description: This catalog contains the evolutionary masses and ages of about 7000 stars in 68 open clusters, as derived from their positions in the theoretical HR diagram. Cluster ages range from 106 to some 109 years, and their population varies from 30 to 700 members. For each cluster we have a table with ages and masses of stars. The file, clusters.dat may include for each cluster, the name (or NGC/IC number), cluster class, assumed color index E(B-V), true distance modulus (V-MV)0, evolutionary tracks used for given cluster and reference to the source of UBV data. The data in data.dat consists of star serial number, color index, V magnitude, luminosity, effective temperature, and ages and masses of stars. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file data.dat 68 9879 Data for individual stars clusters.dat 120 68 General information on each cluster -------------------------------------------------------------------------------- Byte-by-byte Description of file: data.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Cl [1/68]+= Cluster number (see clusters.dat) 4- 6 I3 --- N *Running number within each cluster 10-14 I5 --- ID Star number in UBV source 18-22 F5.3 mag B-V B-V color index 24-29 F6.3 mag Vmag V magnitude 31-32 I2 --- LC Adopted luminosity class 35-39 F5.3 [K] log.Teff Logarithm of effective temperature 41-45 F5.2 [solLum] logL Logarithm of luminosity 48-56 E9.3 yr Age *?=0 Age of the star 58-63 F6.2 solMass Mass ?=0 Mass of the star 66-68 I3 % Prob [0/100] Probability of Age and Mass -------------------------------------------------------------------------------- Note on Age: For stars lying under the ZAMS or to the right of the Hayashi limit, ages are formally defined and are negative, but have no physical meaning. Some stars lie in the forbidden regions of the H-R diagram due to errors of photometry, of conversion procedure, etc. To these stars, reasonable values of age and mass cannot be attributed. In this case, zeros appear in the Age, Mass and Prob fields. Note on N: stars are ordered by absolute magnitudes. -------------------------------------------------------------------------------- Byte-by-byte Description of file: clusters.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Cl [1/68]+= Cluster number (as in data.dat) 5- 8 F4.2 mag E(B-V) Colour excess 10- 14 F5.2 mag m-M *True distance modulus 16 A1 --- Model *[IP] Evolutionary tracks used 18- 36 A19 --- ClName Name of cluster 39-120 A82 --- Ref Reference text -------------------------------------------------------------------------------- Note on m-M: the distance, in parsecs, is: 10(m-M+5) Note on Model: I = Iben I., 1965-67: ApJ 141, 993; 142, 1447; 143, 483; 143, 505; 143, 516; 147, 624; 147, 650 P = Paczinski B., 1970, Acta Astron. 20, 47. -------------------------------------------------------------------------------- Historical notes: * 11-Feb-1997: clusters.dat data file reshaped at CDS
(End) Julie Anne Watko [SSDOO/ADC] 08-Jan-1997
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