H2O Isotopologues in Extreme OH/IR Stars
- Author(s)
- Kay Justtanont, Michael J. Barlow, Joris A D L Blommaert, Leen Decin, Franz Kerschbaum
- Abstract
Using Herschel Space Observatory, we observed isotopologues of H2O in extreme OH/IR stars. We detected strong H216O and H217O while the H218O lines are missing, contrary to the overall galactic oxygen abundance in the interstellar medium and the Sun, where 18O is more abundant than 17O. Theoretical stellar evolution suggests that 18O is being destroyed during the hot-bottom burning. This implies that these OH/IR stars come from a population of intermediate-mass stars which have an initial mass ≥ 5 M⊙.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Aix-Marseille Université, Chalmers University of Technology, University College London, Katholieke Universiteit Leuven
- Pages
- 85 - 90
- Publication date
- 08-2015
- Austrian Fields of Science 2012
- 103003 Astronomy, 103004 Astrophysics
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/h2o-isotopologues-in-extreme-ohir-stars(10efb29d-53eb-49aa-9f4a-dc117fc919cb).html