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
Last Update 2026-03-02
Keywords Herschel Space Observatory data, ESA Herschel mission dataset, far-infrared astronomy observations, submillimeter astronomy data, infrared space telescope observations, PACS photometer data, PACS spectrometer data, SPIRE photometer data, SPIRE Fourier transform spectrometer data, HIFI heterodyne spectroscopy data, far-infrared spectroscopy dataset, submillimeter spectral line observations, cold universe observations dataset, star formation infrared data, molecular cloud far-infrared observations, interstellar medium spectroscopy data, protoplanetary disk infrared observations, galaxy evolution far-infrared data, dust emission submillimeter observations, cosmic infrared background measurements, extragalactic infrared survey data, calibrated level 2 data products, FITS files astronomy, spectral cubes far-infrared, flux-calibrated maps, continuum photometry data, spectral energy distribution measurements, ESA Herschel Science Archive data
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