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- W2807745543 abstract "We recalculated the distance to 554 galactic Planetary Nebulae (PNe) using the relation between the ionized mass of the nebula μ and the optical thickness parameter τ obtained by Akimkin et al. [1]. We classified these nebulae according to the Peimbert [9] types modified by Quireza et al. [11]. The obtained by us distances to galactic PNe were used to obtain the scale heights h for different subsystem of the Milky Way. Next values if h were estimated: h = 208 ± 10 pc for thin disk objects, h = 600 ± 54 pc for thick disk ones, and h = 1378 ± 180 pc for halo PNe." @default.
- W2807745543 created "2018-06-21" @default.
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- W2807745543 date "2018-06-01" @default.
- W2807745543 modified "2023-09-25" @default.
- W2807745543 title "The spatial structure of the Galaxy subsystems as it looks from an analysis of the system of galactic planetary nebulae" @default.
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- W2807745543 doi "https://doi.org/10.1088/1742-6596/1038/1/012016" @default.
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