A dataset provided by the European Space Agency

Name OT2_pcrowthe_2
Title Oxygen abundances in carbon-type Wolf-Rayet stars from PACS scan spectroscopy
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342247822&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342252252&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342252269&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342257690&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342257695&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-rg3i0z4
Author crowther, p.
Description This is a resubmitted priority 2 OT1 programme to scan OIII 88micron with PACS for a sample of Milky Way carbon and oxygen sequence Wolf-Rayetstars. The proposed observations, requiring 7.7hr will: (i) enable reliableoxygen abundances to be determined for WC stars for the first time, testingevolutionary predictions; (ii) refine the degree of clumping in the outerstellar winds of these stars derived from existing ISO/SWS or Spitzer/IRSdatasets. The requested line spectra are unique to PACS and cannot beacquired with another instrument for these targets.
Publication
    Instrument PACS_PacsRangeSpec_point
    Temporal Coverage 2012-07-10T14:45:40Z/2012-12-23T13:03:41Z
    Version SPG v14.2.0
    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 2013-06-23T09:06:32Z
    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, crowther et al., 2013, 'Oxygen abundances in carbon-type Wolf-Rayet stars from PACS scan spectroscopy', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-rg3i0z4