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An observational study of dust nucleation in Mira (o Ceti) I. Variable features of AlO and other Al- bearing species
| Indexado |
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| DOI | 10.1051/0004-6361/201628664 | ||||
| Año | 2016 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
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.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Kaminski, Tomasz | Hombre |
ESO - Chile
European Southern Observatory Santiago - Chile |
| 2 | Wong, Ka Tat | - |
Max Planck Inst Radioastron - Alemania
Max Planck Institute for Radio Astronomy - Alemania |
| 3 | MORA-FERNANDEZ, ALCIONE | Hombre |
Polish Acad Sci - Polonia
Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences - Polonia |
| 4 | Müller, Holger S.P. | - |
Inst Phys 1 - Alemania
University of Cologne - Alemania Universität zu Köln - Alemania |
| 5 | Gottlieb, C. A. | - |
Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos |
| 6 | Cherchneff, I. | - |
UNIV BASEL - Suiza
Universitat Basel - Suiza |
| 7 | Menten, K. M. | Hombre |
Max Planck Inst Radioastron - Alemania
Max Planck Institute for Radio Astronomy - Alemania |
| 8 | KELLER-DIAZ, ANDRES | Hombre |
Max Planck Inst Radioastron - Alemania
Max Planck Institute for Radio Astronomy - Alemania |
| 9 | Brünken, S. | Mujer |
Inst Phys 1 - Alemania
University of Cologne - Alemania Universität zu Köln - Alemania |
| 10 | Winters, J. M. | Hombre |
IRAM - Francia
IRAM Institut de RadioAstronomie Millimétrique - Francia Universite Grenoble Alpes - Francia |
| 11 | Patel, Nimesh | - |
Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos |
| Agradecimiento |
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| We thank T. Kipper (Tartu Observatory) for sending us a copy of his article. We are also grateful to O. Adriyenko (Terskol Observatory) for providing us with his spectra and E. Griffin (NRC-Herzberg) for her efforts to digitalize the DAO spectroscopical plates. We acknowledge with thanks the variable star observations from the AAVSO International Database contributed by observers worldwide and used in this research. Based on data obtained from the ESO Science Archive Facility and made with ESO Telescopes at the La Silla Paranal Observatory under programme IDs 074.D-0114(A) and 089.D-0383(A). Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientique of France, and the University of Hawaii. Based on observations obtained at the Dominion Astrophysical Observatory, NRC Herzberg, Programs in Astronomy and Astrophysics, National Research Council of Canada. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. This research has made use of the Keck Observatory Archive (KOA), which is operated by the W. M. Keck Observatory and the NASA Exoplanet Science Institute (NExScI), under contract with the National Aeronautics and Space Administration. Based on analysis carried out with the CASSIS software and JPL spectroscopic database. CASSIS has been developed by IRAP-UPS/CNRS (http://cassis.irap.omp.eu). This paper makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.00014.SV, 2013.1.00047.S, 2012.1.00524.S, 2013.1.00156.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. |
