J/A+AS/124/353      CCD UBV photometry of close visual doubles (Nakos+ 1997)

UBV absolute CCD photometry and differential astrometry of close visual double stars, with G-type primaries. Nakos T., Sinachopoulos D., van Dessel E. <Astron. Astrophys. Suppl. Ser. 124, 353 (1997)> =1997A&AS..124..353N 1997A&AS..124..353N (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Photometry, CCD ; Photometry, UBV Keywords: binaries: visual - catalog Abstract: We present V magnitudes, (B-V) and (U-B) colours of close visual double star components, and their differences as well as separations and position angles of 40 visual double stars. The common properties of the members of this sample are the small angular separation ρ, which is less than 7", and the common spectral type of the primaries, which are of G-type. The observations made with the Bessel U, B and V filters, while the astrometry was performed in the V filter only. For the observations, the CCD camera attached to the Cassegrain focus of the 90 cm Dutch telescope, at La Silla, Chile, had been used. From the analysis of the data we concluded that from the sample of the fourty double stars observed seven proved to be physical pairs, while the rest must have common origin components. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1 58 39 Astrometric results table2 45 80 Photometric results table3 38 40 Photometric differences and angular separation of the components tables.tex 78 313 LaTeX version of the tables -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- No Visual binary number 5- 6 I2 h RAh Right ascension (J2000) 8- 11 F4.1 min RAm Right ascension (J2000) 13 A1 --- DE- Declination sign 14- 15 I2 deg DEd Declination (J2000) 17- 18 I2 arcmin DEm Declination (J2000) 20- 28 A9 --- DM Durchmusterung designation of the primary 30- 34 F5.3 arcsec rho Angular separation 36- 39 F4.3 arcsec e_rho rms uncertainty on rho (1) 41- 47 F7.3 deg Theta Position angle 49- 51 F3.2 deg e_Theta rms uncertainty on Theta 53- 58 F6.1 yr Obs Epoch of observation -------------------------------------------------------------------------------- Note (1): The very small values of e_rho are due to the assumption of σr(ρ)=0. We took σr(ρ)=0 for the error of the angular separation rho due to the atmospheric refraction. Realistic values of e_rho are probably one order of magnitude higher -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- No Visual binary number 4- 12 A9 --- DM DM number 13 A1 --- m_DM Multiplicity index on DM 15- 20 F6.3 mag Vmag V magnitude 22- 24 F3.2 mag e_Vmag rms uncertainty on Vmag 26- 30 F5.3 mag B-V B-V colour index 32- 34 F3.2 mag e_B-V rms uncertainty on B-V 36- 41 F6.3 mag U-B U-B colour index 43- 45 F3.2 mag e_U-B rms uncertainty on U-B -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- No Visual binary number 4- 12 A9 --- DM DM or ADS number 14- 18 F5.3 arcsec rho ? Angular separation 20- 24 F5.3 mag DVmag Difference in V magnitude 26- 31 F6.3 mag D(B-V) Difference in B-V colour index 33- 38 F6.3 mag D(U-B) Difference in U-B colour index -------------------------------------------------------------------------------- Acknowledgements: Dimitris Sinachopoulos
(End) Patricia Bauer [CDS] 03-Dec-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