J/A+AS/104/379    Integrated Photometry of open clusters      (Battinelli+ 1994)

Integrated photometric properties of open clusters BATTINELLI P., BRANDIMARTI A., CAPUZZO-DOLCETTA R. <Astron. Astrophys. Suppl. Ser. 104, 379 (1994)> =1994A&AS..104..379B 1994A&AS..104..379B
Keywords: clusters: open and associations - techniques: photometric ADC_Keywords: Clusters, open; Photometry Abstract: Galactic open clusters provide an abundant sample of stellar aggregates of various sizes, ages and metal abundances, apt to constitute a template for comparison with star systems in other galaxies. In this paper we present and discuss a standard methodology to synthesize U,B,V fluxes and colours, and apply it to a set of 138 open clusters. Results are compared with previous ones available in the literature. We were able to calibrate a mass-luminosity relation by which we evaluated the mass of ∼ 400 open clusters, leading to a well defined present-day mass function. The number-complete sample of galactic open clusters presented in Battinelli & Capuzzo-Dolcetta (1992AJ....103.1596B 1992AJ....103.1596B) is enlarged of a 15%. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 62 138 Magnitude, colour and mass refs.dat 93 106 References to table1 table2.dat 65 115 Galactic coordinates, distance and age -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name *Open cluster name 9- 12 I4 --- n Number of members stars 13- 18 F6.2 mag Mv Integrated magnitude 20- 24 F5.2 mag (B-V)0 (B-V)0 colour in decimal log 26- 30 F5.2 mag (U-B)0 ? (U-B)0 colour in decimal log 32- 35 F4.2 [solMass] logM Mass in decimal log 37- 42 A6 --- Notes *Notes on integrated photometry 43- 62 A20 --- r_Notes Comma-separated references, see file refs.dat -------------------------------------------------------------------------------- Note on Name: Bas=Basel, Ber=Berkeley, Bla=Blanco, Boc=Bochum, Byu=Byurakan, Col=Collinder, Fei=Feinstein, Hog=Hogg, Hya=Hyades, Lyn=Lynga, Mar=Markarian, N=NGC, Pis=Pismis, Ple=Pleiades, Ros=Roslund, Rup=Ruprecht, Tra=Trapezium, Upg=Upgren, VdH=van den Bergh & Hagen, Wat=Waterloo, Wes=Westerlund. Note on Notes: The symbols refer to other authors who give integrated photometry: b= Spassova N.M. & Baev P.V. =1985Ap&SS.112..111S 1985Ap&SS.112..111S g= Gray D.F. =1965AJ.....70..362G 1965AJ.....70..362G l= Lynga G. 1987, Lund Catalogue of Open Cluster Data, 5th ed., CDS Catalogue V/92 p= Pandey A.K., Bhatt B.C., Mahra H.S. & Sagar R. =1989MNRAS.236..263P 1989MNRAS.236..263P s= Sagar R., Joshi U.C. & Sinvhal S.D. 1983, Bull. Astron. Soc. India 11, 44 Symbol c stands for clusters in the "complete" sample and symbol : stands for uncertain values. Hog 17 is included in the sample due to BCD determination based on a higher number of members (41). ------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- RefNo [1,106]+ Reference number 5- 23 A19 --- BibCode Coded Reference 25- 93 A69 --- Text Text of reference -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name *Open cluster name 10- 15 F6.2 deg GLON Galactic longitude l 17- 22 F6.2 deg GLAT Galactic latitude b 24- 27 I4 pc d Projected distance to the Sun 29- 35 F7.2 pc z Height on the galactic plane 37- 41 F5.1 arcmin D Angular diameter 45- 48 F4.2 [yr] Log(t) ? Logarithmic age 53- 57 F5.2 mag (B-V)to ? Turn-off colour 61- 64 F4.2 mag E(B-V) Reddening -------------------------------------------------------------------------------- Note on Name: Bas=Basel, Ber=Berkeley, Bla=Blanco, Boc=Bochum, Byu=Byurakan, Col=Collinder, Fei=Feinstein, Hog=Hogg, Hya=Hyades, Lyn=Lynga, Mar=Markarian, N=NGC, Pis=Pismis, Ple=Pleiades, Ros=Roslund, Rup=Ruprecht, Tra=Trapezium, Upg=Upgren, VdH=van den Bergh & Hagen, Wat=Waterloo, Wes=Westerlund. -------------------------------------------------------------------------------- History: * 18-Jan-1994: first archived at CDS (Patricia Bauer) * 24-Jan-1999: references added (Francois Ochsenbein)
(End) Patricia Bauer, Francois Ochsenbein [CDS] 24-Jan-1999
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