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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...

Deskribapen osoa

Gorde:
Xehetasun bibliografikoak
Egile Nagusiak: Owen Chase, Robin Ciardullo, Martin M. Roth, George H. Jacoby
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: IOP Publishing 2023-01-01
Saila:The Astrophysical Journal
Gaiak:
Sarrera elektronikoa:https://doi.org/10.3847/1538-4357/acc9bd
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