Water masers in post-AGB and planetary nebulae. A special category of evolved sources?

Physics

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Stellar, Galactic, Parkes

Scientific paper

Water masers are present in evolved stars, but until 2001 it was thought that they could not be found in planetary nebulae (PNe). We propose to carry out a survey for water maser emission in 106 post-AGB and planetary nebulae selected by their IRAS colours, with declination <-32deg. This is a continuation of our work with NASA's 70m antenna in Spain (for sources with decl > -32deg), in which we observed 109 such sources and detected water maser emission in 2 post-AGB and 4 PNe. This survey in southern sources will help us to confirm the results suggested for the northern ones: a) That the presence of water masers in PNe is not an extremely unlikely event (there are now 5 known cases). b) That post-AGB and PNe with water masers could constitute a special type of evolved objects (still to be defined), probably with massive progenitor stars. c) That water masers could be favoured in PNe over post-AGB stars in this special type of objects.

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