Optical spectrum of the post-AGB star HD56126 in the region 4010-8790 AA

Details Optical spectrum of the post-AGB star HD56126 in the region 4010-8790 AA Optical spectrum of the post-AGB star HD56126 in the region 4010-8790 AA

2007-04-05

arxiv.org/abs/0704.0677v1

Astrophys.Bull.62:162-192,2007

Astronomy and Astrophysics

Astrophysics

42 pages, 6 figures

Scientific paper

10.1134/S199034130702006X

We studied in detail the optical spectrum of the post-AGB star HD56126 (IRAS07134+1005). We use high resolution spectra (R=25000 and 60000) obtained with the echelle spectrographs of the 6-m telescope. About one and a half thousand absorptions of neutral atoms and ions, absorption bands of C_2, CN, and CH molecules, and interstellar bands (DIBs) are identified in the 4010 to 8790 AA wavelength region, and the depths and radial velocities of these spectral features are measured. Differences are revealed between the variations of the radial velocities measured from spectral features of different excitation. In addition to the well-known variability of the Halpha profile, we found variations in the profiles of a number of FeII, YII, and BaII lines. We also produce an atlas of the spectrum of HD56126 and its comparison staralpha Per. The full version of the atlas is available in electronic form from Web-address: http://www.sao.ru/hq/ssl/Atlas/Atlas.html

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