Scandium and chromium in the strontium filament in the Homunculus of η Carinae

• Published in: Monthly notices of the Royal Astronomical Society Vol. 393; no. 4; pp. 1503 - 1512
• Main Authors: Bautista, M. A., Ballance, C., Gull, T. R., Hartman, H., Lodders, K., Martínez, M., Meléndez, M.
• Format: Journal Article
• Language: English
• Published: Oxford, UK Blackwell Publishing Ltd 11.03.2009; Wiley-Blackwell
• Subjects: Astronomy; atomic data; atomic processes; Earth, ocean, space; Exact sciences and technology; line: formation; stars: abundances; atomic processes; line: formation; atomic data; stars: abundances; Radiative transition; Electron impact excitation; Atomic process; Line formation; Stellar abundance; Thermodynamic non equilibrium; Filaments; Emission spectra; Models; Abundance ratio; Ab initio calculations; Rate constant; Electron density; LTE
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1111/j.1365-2966.2008.14246.x

We continue a systematic study of chemical abundances of the strontium filament found in the ejecta of η Carinae. To this end we interpret the emission spectrum of Sc ii and Cr ii using multilevel non-local thermodynamic equilibrium models. Since the atomic data for these ions were previously unavailable, we carry out ab initio calculations of radiative transition rates and electron impact excitation rate coefficients. The observed spectrum is consistent with an electron density of the order of 107 cm−3 and a temperature between 6000 and 7000 K, conditions previously determined from [Ni ii], [Ti ii] and [Sr ii] diagnostics. The observed spectrum indicates an abundance of Sc relative to Ni more than 40 times the solar value, while the Cr/Ni abundance ratio is roughly solar. Various scenarios of depletion and dust destruction are suggested to explain such abnormal abundances.