A dataset provided by the European Space Agency

Name OT1_pcrowthe_1
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=1342211677&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342262042&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI 10.5270/esa-pocs5x1
Author crowther, p.
Description We seek 13.6 hours of spectral scans of the [OIII] 88 micron fine-structure line with PACS for a sample of Milky Way carbon and oxygen sequence Wolf-Rayet stars. The proposed observations will: (i) enable reliable oxygen abundances to be determined for WC stars for the first time, to test evolutionary predictions; (ii) refine the degre of clumpig in the outer stellar winds of these stars derived from existing ISO-SWS or Spitzer-IRS datasets.
Publication
Instrument PACS_PacsRangeSpec_point
Temporal Coverage 2010-12-24T14:13:01Z/2013-01-26T03:13:32Z
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 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-07-26T01:54:09Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-07-26T01:54:09Z, OT1_pcrowthe_1, SPG v14.2.0. https://doi.org/10.5270/esa-pocs5x1