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Table B.2
New, reobserved, and mis-classified PNe with emission-line central stars.
Name | FWHM | Classification | |||
t.w. | WG | ||||
|
|||||
New WELs: | |||||
PB 5 | WEL | – | |||
My 60 | WEL? | – | |||
He 2-115 | WEL | – | |||
New [WR]: | |||||
He 2- 67 | 43 Å | [WC 4] | – | ||
He 2-117 | 25 Å | [WC 5-6] | – | ||
He 2-125 | VL | – | |||
Reobserved: | |||||
Pe 1- 1 | 45 Å | [WC 4-5] | [WO 4] | ||
He 2- 63 | undetect. | WEL | |||
He 2- 86 | 22 Å | [WC 5-6] | [WC 4] | ||
He 2-107 | VL | [WC10-11] | |||
He 2-131 | VL | WEL | |||
He 2-108 | VL | WEL | |||
He 2-123 | WEL | WEL? | |||
Misclassified/mimics: | |||||
NGC 6326 | WEL? | ||||
NGC 5979 | not stellar | WEL | |||
NGC 3918 | not stellar | – |
Notes. Column 3 gives the width of C IV λ5805 stellar emission feature if is broader than instrumental profile. Columns 4 and 5 give stellar classification of this work and from Weidmann & Gamen (2011).
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