J/A+A/367/199       UBVR photometry of AX Per                (Skopal+, 2001)

A photometric and spectroscopic study of the eclipsing symbiotic binary AX Persei Skopal A., Teodorani M., Errico L., Vittone A.A., Ikeda Y., Tamura S. <Astron. Astrophys. 367, 199 (2001)> =2001A&A...367..199S 2001A&A...367..199S
ADC_Keywords: Photometry, UBVRI ; Spectroscopy ; Stars, variable Keywords: stars: binaries: symbiotics - stars: circumstellar matter - stars: mass-loss Description: Table 2 presents standard broad band U, B, V, R photoelectric photometry of AX Persei. Each value represents the average of the observations during a night. The uncertainty of these night-means is of a few x 0.001mag in the B, V and R bands, and up to 0.02mag in the U band. Table 3 presents observed spectrophotometric parameters of the spectrum: the line fluxes, fluxes in the local continuum and the radial velocities. Objects: ---------------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------------- 01 36 22.8 +54 15 02 AX Per = MWC 411 = HV 5488 ---------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 39 244 Johnson U, B, V, R photometry table3.dat 88 54 Spectrophotometric parameters -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 F11.3 d JD [2447860/2451511] Julian date 13- 18 F6.3 mag Umag ? U magnitude 20- 25 F6.3 mag Bmag ? B magnitude 27- 32 F6.3 mag Vmag ? V magnitude 34- 39 F6.3 mag DRmag ? Delta R magnitude = AX Per - S1 (1) -------------------------------------------------------------------------------- Note (1): DR = AX Per - S1 in the filter R, S1 = HD 9839 (BD+54331, SAO 22444) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- Element Element (1) 9- 16 F8.3 0.1nm lambda Wavelength 18- 21 F4.1 mW/m2 Flux ? 13.Oct.1992 flux in the line (2) 23- 26 F4.1 10mW/m2/nm I ? 13.Oct.1992 height of the line above the local continuum Fc (2) 28- 30 F3.1 10mW/m2/nm Fc ? 13.Oct.1992 local continuum (2) 32- 37 F6.1 km/s RV ? 13.Oct.1992 radial velocity 39 A1 --- m/p [mp?] 13.Oct.1992 flag on mid (m) and peak (p) of line 41- 45 F5.1 mW/m2 Flux2 ? 09.Jan.1998 flux in the line (2) 46 A1 --- u_Flux2 [?] ? for unknown value 47- 51 F5.1 10mW/m2/nm I2 ? 09.Jan.1998 height of the line above the local continuum Fc (2) 53- 55 F3.1 10mW/m2/nm Fc2 ? 09.Jan.1998 local continuum (2) 57- 62 F6.1 km/s RV2 ? 09.Jan.1998 radial velocity 64 A1 --- m/p2 [mp?] 09.Jan.1998 flag on mid (m) and peak (p) of line 66- 70 F5.1 mW/m2 Flux3 ? 05.Sep.1998 flux in the line (2) 72- 75 F4.1 10mW/m2/nm I3 ? 05.Sep.1998 height of the line above the local continuum Fc (2) 77- 79 F3.1 10mW/m2/nm Fc3 ? 05.Sep.1998 local continuum (2) 81- 86 F6.1 km/s RV3 ? 05.Sep.1998 radial velocity 88 A1 --- m/p3 [mp?] 05.Sep.1998 flag on mid (m) and peak (p) of line -------------------------------------------------------------------------------- Note (1): For FeI abs: RV = -116.8 ± 2.4 km/s for 11 lines, 13 Oct 1992 observation RV = -128.5 ± 0.9 km/s for 29 lines, 09 Jan 1998 observations RV = -111.5 ± 1.3 km/s for 41 lines, 05 Sep 1998 observations Note (2): 10mW/m2/nm = erg/cm2/s/Å ; mW/m2 = erg/cm2/s -------------------------------------------------------------------------------- Acknowledgements: Augustin SKOPAL
(End) Patricia Bauer [CDS] 05-Jan-2001
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