| 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 |
| DOI | https://doi.org/10.5270/esa-pocs5x1 |
| Author | European Space Agency |
| 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 µm range, bridging the gap between earlier infrared space missions and groundbased facilities. |
| Creator Contact | https://support.cosmos.esa.int/h®erschel/ |
| Date Published | 2013-07-26T01:54:09Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 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-pocs5x1 |