edoc

An observational study of dust nucleation in Mira (o Ceti). I. Variable features of AlO and other Al-bearing species

Kamiński, T. and Wong, K. T. and Schmidt, M. R. and Müller, H. S. P. and Gottlieb, C. A. and Cherchneff, I. and Menten, K. M. and Keller, D. and Brünken, S. and Winters, J. M. and Patel, N. A.. (2016) An observational study of dust nucleation in Mira (o Ceti). I. Variable features of AlO and other Al-bearing species. Astronomy and Astrophysics, 592. A42.

[img]
Preview
PDF - Published Version
5Mb

Official URL: http://edoc.unibas.ch/53885/

Downloads: Statistics Overview

Abstract

Context: Dust is efficiently produced by cool giant stars, but the condensation of inorganic dust is poorly understood. Observations of key aluminum bearing molecules around evolved stars has enabled us to investigate the nucleation of alumina (Al 2 O 3 ) dust in the gas.
Aims: We aim to identify and characterize aluminum bearing species in the circumstellar gas of Mira (o Ceti) in order to elucidate their role in the production of Al 2 O 3 dust. Methods: We used multiepoch spectral line observations at (sub-)millimeter, far-infrared, and optical wavelengths including: maps with ALMA that probe the gas distribution in the immediate vicinity of the star at ~30 mas; observations with ALMA, APEX, and Herschel in 2013-2015 for studying cycle and inter-cycle variability of the rotational lines of Al-bearing molecules; optical records as far back as 1965 to examine variations in electronic transitions over time spans of days to decades; and velocity measurements and excitation analysis of the spectral features that constrain the physical parameters of the gas.
Results: Three diatomic molecules AlO, AlOH, and AlH, and atomic Al i are the main observable aluminum species in Mira, although a significant fraction of aluminum might reside in other species that have not yet been identified. Strong irregular variability in the (sub-)millimeter and optical features of AlO (possibly the direct precursor of Al 2 O 3 ) indicates substantial changes in the excitation conditions, or varying abundance that is likely related to shocks in the star. The inhomogeneous distribution of AlO might influence the spatial and temporal characteristics of dust production.
Conclusions: We are unable to quantitatively trace aluminum depletion from the gas, but the rich observational material constrains time-dependent chemical networks. Future improvements should include spectroscopic characterization of higher aluminum oxides, coordinated observations of dust and gas species at different variability phases, and tools to derive abundances in shock-excited gas. The ALMA data, including spectral cubes, moment-zero maps, and spectra, are only available at the CDS via anonymous ftp to  http://cdsarc.u-strasbg.fr ( http://130.79.128.5 ) or via  http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/592/A42
Faculties and Departments:05 Faculty of Science > Departement Physik > Former Organization Units Physics > Theoretische Physik Astrophysik (Thielemann)
UniBasel Contributors:Cherchneff-Parrinello, Isabelle
Item Type:Article, refereed
Article Subtype:Research Article
Publisher:EDP Sciences
ISSN:0004-6361
e-ISSN:1432-0746
Note:Publication type according to Uni Basel Research Database: Journal article
Language:English
Identification Number:
Last Modified:01 Mar 2017 07:57
Deposited On:20 Feb 2017 12:09

Repository Staff Only: item control page