A systematic infrared analysis of PG1159 planetary nebulae finds cooler dust and lower dust masses than other hydrogen-poor nebulae and suggests an evolutionary sequence from [WRE] to PG1159 central stars based on H beta surface brightness.
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Infrared properties of Planetary Nebulae with PG1159 central stars
A systematic infrared analysis of PG1159 planetary nebulae finds cooler dust and lower dust masses than other hydrogen-poor nebulae and suggests an evolutionary sequence from [WRE] to PG1159 central stars based on H beta surface brightness.