J/A+A/339/165 The red spectrum of HD 101065 (Cowley+ 1998)
Line identifications and preliminary abundances
from the red spectrum of HD 101065 (Przybylski's star)
Cowley C.R., Mathys G.
<Astron. Astrophys. 339, 165 (1998)>
=1998A&A...339..165C 1998A&A...339..165C (SIMBAD/NED BibCode)
ADC_Keywords: Stars, peculiar ; Spectra, red ; Abundances, peculiar
Keywords: stars: individual: HD 101065 - stars: abundances -
stars: chemically peculiar - stars: magnetic fields
Description:
Wavelength list for Przybylski's star (a rapidly rotation Ap star)
including a measurement of the line depths.
Objects:
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RA (2000) DE Designation(s)
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11 37 37.2 -46 42 37 HD 101065 = Przybylski's star
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File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table2.dat 104 1066 Wavelength list for Przybylski's star
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Byte-by-byte Description of file: table2.dat
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Bytes Format Units Label Explanations
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1- 7 F7.2 0.1nm Lambda Measured wavelength
9- 12 F4.2 --- Int Measured central intensity (1)
14- 15 I2 --- Strength Line strength (2)
16 A1 --- n_Strength [:] : when eye estimates
19- 42 A24 --- Id1 First identification (3)
43- 66 A24 --- Id2 Second identification (3)
67- 90 A24 --- Id3 Third identification (3)
91-114 A24 --- Id4 Fourth identification (3)
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Note (1): Central depth of the line, as measured from a convolved and
Fourier filtered spectrum (1.00 corresponds to the continuum level).
Note (2): Estimate of the line strength on an arbitrary scale, derived
from the measured line depth. Intensities of lines in the wing of
Hα are eye estimates, and not computed from the line depths.
They are given with colons
Note (3): Up to 4 possible contributing transitions are identified for
the measured lines. The fractional part of the laboratory wavelength
of the transition is given, followed by spectrum (e.g. Nd II). For
most of the lanthanide spectra, the parenthesized number following the
spectrum is the intensity from Meggers, Corliss, and Scribner (NBS
Monog. 145, 1975). Iron-group spectra are typically followed by
Multiplet numbers (e.g. Fe I-15 is a line from Multiplet 15). Energy
levels are sometimes given for third spectra of the lanthanides.
These are from Martin, Zalubas, and Hagan (NSRDS-NBS 60, 1978), or
unpublished material provided to CRC by Hannah Crosswhite. Lines
lacking energy-level classifications are designated "uncl."
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Acknowledgements: Gautier Mathys
(End) G. Mathys (ESO, Santiago, Chile), Patricia Bauer [CDS] 28-Sep-1998