SOFIA observations of the planetary nebula NGC 7009
We report spectrophotometric observations made with SOFIA/FORCAST on 2011 June 2 UT. Optical measurements have previously shown that the abundance discrepancy factor (adf) varies with position in several high-adf PNe, and is highest close to the central star. The very low electron temperature inclus...
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| Veröffentlicht in: | Proceedings of the International Astronomical Union 2011-07, Vol.7 (S283), p.67-70 |
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| container_issue | S283 |
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| container_title | Proceedings of the International Astronomical Union |
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| creator | Rubin, R. H. Colgan, S. W. J. Corradi, R. L. M. Sankrit, R. Tielens, A. G. G. M. Tsamis, Y. G. Sivaraja, V. |
| description | We report spectrophotometric observations made with SOFIA/FORCAST on 2011 June 2 UT. Optical measurements have previously shown that the abundance discrepancy factor (adf) varies with position in several high-adf PNe, and is highest close to the central star. The very low electron temperature inclusions postulated to explain the abundance discrepancy, must be cooled predominantly by fine structure IR lines. These SOFIA data will map mid-IR FS lines (and our related Herschel program will add several far-IR FS lines) in the bright, well-characterized, high-adf PN NGC 7009. We will compare these IR results with FS optical line measurements in order to correlate ratios of IR to optical fluxes with position, and thus correlate with where the adf peaks. |
| doi_str_mv | 10.1017/S174392131201071X |
| format | Article |
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These SOFIA data will map mid-IR FS lines (and our related Herschel program will add several far-IR FS lines) in the bright, well-characterized, high-adf PN NGC 7009. 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| subjects | Abundance Astronomical instruments Astrophysics Contributed Papers Correlation analysis Electron temperature Fine structure Fluxes Infrared radiation Nebulae Optical measurement Stars & galaxies |
| title | SOFIA observations of the planetary nebula NGC 7009 |
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