Isotopic abundance of carbon in the DLA towards QSO B1331+170

Autor(en)
Dinko Milaković, John Webb, Paolo Molaro, Lee Chung-Chi, Prashin Jethwa, Guido Cupani, Michael T. Murphy, Louise Welsh, Valentina D'Odorico, Stefano Cristiani, Ricardo Génova Santos, C. J. A. P. Martins, Nelson J Nunes, Tobias Marius Schmidt, Francesco A Pepe, Maria Rosa Zapatero Osorio, Yann Alibert, J I González Hernández, Paolo Di Marcantonio, Enric Palle, Rafael Rebolo, Nuno C Santos, S. G. Sousa, Alejandro Suárez Mascareño
Abstrakt

Chemical evolution models predict a gradual build-up of 13C in the Universe, based on empirical nuclear reaction rates and assumptions on the properties of stellar populations. However, old metal-poor stars within the Galaxy contain more 13C than is predicted, suggesting that further refinements to the models are necessary. Gas at high-redshift provides important supplementary information at metallicities −2≲[Fe/H]≲−1, for which there are only a few measurements in the Galaxy. We obtained new, high-quality, VLT/ESPRESSO observations of the QSO B1331+170 and used them to measure 12C/13C in the damped Lyman-α system (DLA) at zabs=1.776, with [Fe/H] = -1.27. AI-VPFIT, an artificial intelligence tool based on genetic algorithms and guided by a spectroscopic information criterion, was used to explore different possible kinematic structures of the carbon gas. Three hundred independent AI-VPFIT models of the absorption system were produced using pre-set 12C/13C values, ranging from 4 to 500. Our results show that 12C/13C=28.5+51.5−10.4, suggesting a possibility of 13C production at low metallicity.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Institute for Fundamental Physics of the Universe, INAF Astronomical Observatory of Triest, University of Cambridge, Big Questions Institute, Swinburne University of Technology, Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Trieste, Instituto de Astrofísica de Canarias (IAC), Universidad de La Laguna, Universidade do Porto, Universidade de Lisboa, Universität Genf, Centro de Astrobiología (CSIC-INTA), Universität Bern
Journal
Monthly Notices of the Royal Astronomical Society
Band
534
Seiten
12-29
Anzahl der Seiten
18
ISSN
0035-8711
DOI
https://doi.org/10.1093/mnras/stae2056
Publikationsdatum
10-2024
Peer-reviewed
Ja
ÖFOS 2012
103004 Astrophysik
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/d1bed1f9-ddc7-4955-8a38-2d5f1eda87fd