The Effect of Superpositions on the Planetary Nebula Luminosity Function
Planetary nebula (PN) surveys in systems beyond ∼10 Mpc often find high-excitation, point-like sources with [O iii ] λ 5007 fluxes greater than the apparent bright-end cutoff of the planetary nebula luminosity function (PNLF). Here we identify PN superpositions as one likely cause for the phenomenon...
मुख्य लेखकों: | , , , |
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स्वरूप: | लेख |
भाषा: | English |
प्रकाशित: |
IOP Publishing
2023-01-01
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श्रृंखला: | The Astrophysical Journal |
विषय: | |
ऑनलाइन पहुंच: | https://doi.org/10.3847/1538-4357/acc9bd |