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J/A+A/506/845       Line list of HD 143418     (Zverko+, 2009)

The puzzling binary HD 143418. Zverko J., Ziznovsky J., Mikulasek Z., Krticka J., Iliev I.K., Stateva I.K., Romanyuk I.I., Kudryavtsev D.O. <Astron. Astrophys., 506, 845-856 (2009)> =2009A&A...506..845Z
ADC_Keywords: Atomic physics Keywords: binaries: spectroscopic - stars: variables: general - stars: chemically peculiar - stars: abundances - stars: evolution - stars: individual HD 143418 Abstract: HD 143418 was discovered recently to be a double-lined spectroscopic binary with a primary designated as a CP star. Its light displays an orbital phase coupled variability with a peak-to-peak amplitude up to 0.04mag. The photometry available and new high dispersion spectra were investigated from a point of view of CP characteristics. A series of high resolution high S/N coude spectra was acquired from which 25 weak to strong unblended lines of Fe I and II, Ti II, Cr II, Zr II, and Ba II were selected to study spectral line variability. Two Zeeman spectra were obtained to search for a possible magnetic field of the star, and one echelle spectrum in a wide spectral region was analysed for abundance determination by means of synthetic spectra. The photometric observations were subjected to a PCA disentangling of the complex photometric behaviour. Description: The twenty-nine spectra from the National Astronomical Observatory, Rozhen, Bulgaria (NAO), were recorded using the photometric AT200 CCD camera with a SITe SI003AB 1024x1024 detector placed at the 3rd optical camera of the coude spectrograph of the 2m RCC telescope, with R=22000, between 14/06/2005 and 03/05/2009. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 15 58 25.7 +43 12 49 HD 143418 = HIP 78226 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table5.dat 63 130 List of lines used in abundance determination using the Zeeman spectrum table6.dat 63 696 List of lines used in abundance determination using the echelle spectrum
See also: J/A+A/464/263 : UBV photometry of HD 143418 (Bozic+, 2007) Byte-by-byte Description of file: table[56].dat
Bytes Format Units Label Explanations
1- 5 A5 --- Ion Ion 7- 14 A8 --- Abund Abundance factor (1) 17- 24 F8.3 0.1nm Line Line wavelength 26- 31 F6.3 eV EP Energy potential 33- 38 F6.3 [-] loggf Oscillator strength 40- 43 A4 --- r_loggf Reference for loggf when other than VALD values (2) 45- 50 F6.3 [-] loggf2 ? Second value of oscillator strength 52- 55 A4 --- r_loggf2 Reference for loggf2 (2) 57- 63 A7 --- Notes Notes (3)
Note (1): Symbols indicate line strength as follows: vW = very weak W = weak M = medium S = strong vS = very strong Note (2): Source of the gf-value when other than VALD values as follows: KB95 = Kurucz & Bell, 1995, CD ROM 23, http://kurucz.harvard.edu/linelists.html KP75 = Kurucz & Peytremann, 1975, SAO Spec. Report, 362 NIST = NIST Atomic Spectra Database, http://physics.nist.gov/ Note (3): Notes as follows: DNF = does not fit with either gf-value MIO = missing in the observed spectrum blend = two lines of the same species
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 21-Jan-2010
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

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