Tsamis, YG;
Walsh, JR;
Péquignot, D;
Barlow, MJ;
Liu, XW;
Danziger, IJ;
(2006)
Unravelling the chemical inhomogeneity of PNe with VLT FLAMES integral-field unit spectroscopy.
Proceedings of the International Astronomical Union
, 2
(234)
pp. 239-242.
10.1017/S1743921306003036.
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Abstract
Recent weak emission-line long-slit surveys and modelling studies of P Ne have convincingly argued in favour of the existence of an unknown component in the planetary nebula plasma consisting of cold, hydrogen-deficient gas, as an explanation for the long-standing recombination-line versus forbidden-line temperature and abundance discrepancy problems. Here we describe the rationale and initial results from a detailed spectroscopic study of three Galactic PNe undertaken with the VLT FLAMES integral-field unit spectrograph, which advances our knowledge about the small-scale physical properties, chemical abundances and velocity structure of these objects across a two-dimensional field of view, and opens up for exploration an uncharted territory in the study and modelling of PNe and photoionized nebulae in general. © 2006 International Astronomical Union.
Type: | Article |
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Title: | Unravelling the chemical inhomogeneity of PNe with VLT FLAMES integral-field unit spectroscopy |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1017/S1743921306003036 |
Publisher version: | https://doi.org/10.1017/S1743921306003036 |
Language: | English |
Additional information: | This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions. |
UCL classification: | UCL UCL > Provost and Vice Provost Offices UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery.ucl.ac.uk/id/eprint/10097977 |
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