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Paper: |
Identifications of Emission Lines in GHRS Spectra of RR Tel |
Volume: |
154, Cool Stars, Stellar Systems and the Sun: Tenth Cambridge Workshop |
Page: |
1277 |
Authors: |
Jordan, C.; Harper, G. M. |
Abstract: |
Spectra of the symbiotic nova RR Tel, obtained with the Goddard High Resolution Telescope on the Hubble Space Telescope, have been used to make identifications of the emission lines observed. The 2p^4 ^3P2 - ^1D2 transition in Al 6, at 2429.50 AA (lambdaair) has been identified for the first time. The He 2 Paschen series has been extended from the n = 3 to n = 16 transition at 2124.61 AA. Further primary and secondary decays from Fe 2 levels pumped by H Lyman alpha and O 6 have been identified. Lines from levels pumped by Si 3 (1206.51 \AA) and He 2 (1084.98 AA), have also been identified. |
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