Herschel observations of extreme OH/IR stars. The isotopic ratios of oxygen as a sign-post for the stellar mass

Autor(en)

Kay Justtanont, Michael J. Barlow, Joris Blommaert, Leen Decin, Franz Kerschbaum

Abstrakt

Aims: The late stages of stellar evolution are mainly governed by the mass of the stars. Low- and intermediate-mass stars lose copious amounts of mass during the asymptotic giant branch (AGB) which obscure the central star making it difficult to study the stellar spectra and determine the stellar mass. In this study, we present observational data that can be used to determine lower limits to the stellar mass.

Methods: Spectra of nine heavily reddened AGB stars taken by the Herschel Space Observatory display numerous molecular emission lines. The strongest emission lines are due to H₂O. We search for the presence of isotopologues of H₂O in these objects.

Results: We detected the ¹⁶O and ¹⁷O isotopologues of water in these stars, but lines due to H₂¹⁸O are absent. The lack of ¹⁸O is predicted by a scenario where the star has undergone hot-bottom burning which preferentially destroys ¹⁸O relative to ¹⁶O and ¹⁷O. From stellar evolution calculations, this process is thought to occur when the stellar mass is above 5 M_⊙ for solar metallicity. Hence, observations of different isotopologues of H2O can be used to help determine the lower limit to the initial stellar mass.

Conclusions: From our observations, we deduce that these extreme OH/IR stars are intermediate-mass stars with masses of ≥ 5 M_⊙. Their high mass-loss rates of ~ 10-4M_⊙ yr^-1 may affect the enrichment of the interstellar medium and the overall chemical evolution of our Galaxy.

Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.Tables 3, 4 and Appendices are available in electronic form at www.aanda.org

Organisation(en)

Institut für Astrophysik

Externe Organisation(en)

Vrije Universiteit Brussel, Flemish Institute for Technological Research (VITO), Chalmers University of Technology, University College London, Katholieke Universiteit Leuven

Journal

Astronomy & Astrophysics

Band

578

Anzahl der Seiten

38

ISSN

0004-6361

DOI

https://doi.org/10.1051/0004-6361/201526270

Publikationsdatum

06-2015

Peer-reviewed

Ja

ÖFOS 2012

103003 Astronomie, 103004 Astrophysik

Schlagwörter

ASJC Scopus Sachgebiete

Astronomy and Astrophysics, Space and Planetary Science

Link zum Portal

https://ucrisportal.univie.ac.at/de/publications/herschel-observations-of-extreme-ohir-stars-the-isotopic-ratios-of-oxygen-as-a-signpost-for-the-stellar-mass(ebba51be-5c0a-47c2-8e4c-4c75edc58910).html