Long-term spectroscopy of eta Carinae. I. The high and low excitation phases

Details Long-term spectroscopy of eta Carinae. I. The high and low excitation phases Long-term spectroscopy of eta Carinae. I. The high and low excitation phases

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..133..299d&link_type=abstract

Astronomy and Astrophysics Supplement, v.133, p.299-316

Astronomy and Astrophysics

Astrophysics

54

Stars: Emission-Line, Be, Stars: Hertzsprung-Russel (Hr) Diagram, Stars: Individual: Eta Carinae, Binaries: General

Scientific paper

Quantitative measurements of line parameters in the spectrum of eta Carinae are presented for both the broad and narrow line components. A total of 655 spectral features were measured in the spectral range 3850 Angstroms to 11000 Angstroms, giving a comprehensive view of the behavior of atomic transitions ranging from a few to tens of electron volts. The spectrum on the phase of maximum intensity in the high excitation lines (1995) is compared with that on minimum intensity (June 1992), showing that at this phase the high excitation lines disappear but the broad components of low excitation lines strengthens. We reject a number of previous line identifications and propose several new ones, including Fe Ii, [Fe Ii], [Fe Iii], [N Ii], and the near-infrared Ca Ii triplet. Some lines commonly used to diagnose density, temperature, chemical composition, and reddening were found to be blended, urging a revision of the results based on previous data. The existence of double-peaked lines, suggested in previous papers, is ruled out. In the case of hydrogen lines, the apparent double-peaks are shown to be real absorption components. The velocity field in the inner 2\arcsec around the central star shows additional components previously unknown. The phases of high and low excitation in eta Carinae are discussed in light of a recently proposed binary system. We suggest a temperature T ~ 16000 K for the primary star, what indicates that it is close to the beginning of the core helium-burning evolutionary stage. Based on data collected at European Southern Observatory and Laboratorio Nacional de Astrofisica. Table 1 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html

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