A dataset provided by the European Space Agency

Name DDT_kjusttan_3
Title Determination of the initial masses for extreme OH/IR stars using isotopologues of H2O
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342271263&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342271264&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342271265&instrument_name=HIFI&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342271266&instrument_name=HIFI&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-oyh9gfx
Author justtanont, k.
Description A subset of Asymptotic Giant Branch (AGB) stars loses mass at avery high rate. The dust effectively shields the radiation from thecentral star, allowing water-ice to condense onto existingsilicate grains. Through the mass loss process, these starsprovide a siginificant fraction to the gas and dust massreturn to the interstellar medium.These so-called extreme OH/IR stars are thought to originate fromstars with initial mass of 5 solar masses or more. These starsare expcted to experience the process of hot-bottom burning whichpreferentially synthesizes 13C and destroys 18O relative tothe more abundant isotope. From HIFI observations of two of theseobjects, we observed a lack of H2_18O in these objects.Our aim here is to underpin the hypothesis of the high-massprogenitor of these stars by observing three isotopologues of H2Ousing HIFI in six other similar objects. Herschel offers thelast opportunity to observe these lines for years to come.
Publication
  • Herschel observations of extreme OH/IR stars. The isotopic ratios of oxygen as a sign-post for the stellar mass | Justtanont K. et al. | Astronomy & Astrophysics Volume 578 id.A115 38 pp. | 578 | 10.1051\\/0004-6361\\/201526270 | 2015A&A...578A.115J | http://adsabs.harvard.edu/abs/2015A%26A...578A.115J
Instrument HIFI_HifiPoint_dbs
Temporal Coverage 2013-04-29T05:56:39Z/2013-04-29T08:03:34Z
Version SPG v14.1.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth cornerstone mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/h®erschel/
Date Published 2013-10-29T07:38:00Z
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, justtanont et al., 2013, 'Determination of the initial masses for extreme OH/IR stars using isotopologues of H2O', SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-oyh9gfx