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Infrared properties of Planetary Nebulae with PG1159 central stars

astro-ph.SR · 2024-12-16 · conditional · novelty 6.0

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 astro-ph.SR · 2024-12-16 · conditional · none · ref 23

    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.