Search catalogue
J/ApJS/126/461 Equivalent Widths in the Spectrum of Sirius (Zhao+, 2000)
Equivalent Widths in the Spectrum of Sirius Zhao G., Qiu H.M., Chen Y.Q., Li Z.W. <Astrophys. J. Suppl. 126, 461 (2000)> =2000ApJS..126..461Z
ADC_Keywords: Atlases ; Line Profiles ; Stars, early-type Keywords: atlases - line: profiles - stars: early-type - stars: individual (α Canis Majoris) Abstract: The equivalent widths of total 546 lines (26 elements are included) in the spectrum of the bright Am star Sirius from 380 to 930 nm are tabulated. The high-resolution, high signal-to-noise ratio spectrum was obtained with the Coude Echelle Spectrograph attached to the 2.16 m telescope at Beijing Astronomical Observatory (Xinglong, China). Here we also give the results of the equivalent widths comparison between our measurements and those of Strom et al. (=1966ApJ...146..880S) and Sadakane & Ueta (=1989PASJ...41..279S). Table 1. Observation Journal of Sirius: ---------------------------------------------------------------------------- Spectral Range Exposure Time Geocentric Radial Velocity (nm) Obs. Date (s) (km s-1) ---------------------------------------------------------------------------- 386.5-572.1 1997 Feb 18/19 180 12.75 (0.45) 383.3-661.9 1997 Feb 18/19 40+40+30 12.37 (0.96) 378.9-551.6 1997 Feb 18/19 40+40 12.31 (0.82) 380.7-649.3 1997 Feb 18/19 40+40 12.42 (0.93) 623.8-922.7 1999 Apr 01/02 300+300 15.49 (0.52) 624.8-930.4 1999 Apr 01/02 300+300 15.58 (0.69) ---------------------------------------------------------------------------- Objects: ---------------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------------- 06 45 08.9 -16 42 58 Sirius = Alpha CMa = HR 2491 = HD 48915 ---------------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 34 546 Equivalent Widths of Sirius
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 5 A5 --- Ion Element and ionization stage 7- 10 I4 --- Num Multiplet number 12- 20 F9.4 0.1nm Lambda Wavelength 22- 26 F5.2 eV LEP Lower excitation potential 28- 32 F5.1 0.1pm EW Measured equivalent width from Sirius spectrum 34 I1 --- q_EW *Quality of line profile
Note on q_EW: The flags only give readers a rough estimation of line quality. Different people may adopt a slightly different opinion for the choice of flag number. The flag numbers 1-3 are recommended to be used in accurate abundance determinations. 1=perfect 2=good 3=slightly blended 4=mildly blended 5=blended
History: From electronic ApJS edition. References: Abt, 1979 ApJ, 230, 485 =1979ApJ...230..485A Aller, 1942 ApJ, 96, 321 =1942ApJ....96..321A Bell, Dreiling, 1981 ApJ, 248, 1031 =1981ApJ...248.1031B Burkhart, Coupry, Lunel, van't Veer, 1987 A&A , 172, 257 =1987A&A...172..257B Gehlich, 1969 A&A, 3, 169 =1969A&A.....3..169G Griffin, Griffin, 1985 A&A, 149, 437 =1985A&A...149..437G Hui-Bon-Hoa, Burkhart, Alecian, 1997 A&A , 323, 901 =1997A&A...323..901H Jiang, Ground-based Astronomy in Asia 1996 (National Astron. Obs. Japan:Tokyo)Asia , 335 Kohl, 1964a Z. Astrophys. , 60, 115 =1964ZA.....60..115K Kohl, Das Spectrum des Sirius λλ3100-8863 Angstrom 1964b (Inst. Theoretische Physik:Kiel) Kurucz, Furenlid, 1979, Smithsonian Astrophys. Obs. Spec. Rep. 387 Lambert, Roby, Bell, 1982 ApJ, 254, 663 =1982ApJ...254..663L Lane, Lester, 1984 ApJ, 281, 723 =1984ApJ...281..723L Latham, 1969, Smithsonian Astrophys. Obs. Spec. Rep. 321 Moore, A Multiplet Table of Astrophysical Interest 1972 (NBS:revised ed; Boulder) Praderie, Boesgaard, Milliard, Pitois, 1977 ApJ, 214, 130 =1977ApJ...214..130P Rentzsch-Holm, 1997 A&A, 317, 178 =1997A&A...317..178R Rogerson, 1987 ApJS, 63, 369 =1987ApJS...63..369R Sadakane, 1991 PASP, 103, 355 =1991PASP..103..355S Sadakane, Jugaku, Takada-Hidai, 1988 PASP, 100, 811 =1988PASP..100..811S Sadakane, Ueta, 1989 PASJ, 41, 279 =1989PASJ...41..279S Strom, Gingerich, Strom, 1966 ApJ, 146, 880 =1966ApJ...146..880S Wahlgren et al., 1993 BAAS, 25, 1321
(End) Gail L. Schneider [NASA/ADC] 07-Sep-2000
| 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 |
© UDS/CNRS