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Releases: atomneb/WR_PN_Chemistry_Data

WR-PN-Chemistry-Data.1.2

26 Aug 02:36
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Physical and chemical properties of Wolf-Rayet planetary nebulae. Supplementary Data

Table 4 lists observed and dereddened line fluxes on a scale relative to Hb, where Hb = 100.

Table 6 presents electron temperatures and densities derived from CELs.

Table 7 presents electron temperatures derived from He I lines.

Table 8 presents electron temperatures and densities derived from ORLs.

Table 11 presents ionic abundances relative to hydrogen derived from CELs.

Table 12 presents ionic abundances relative to hydrogen derived from ORLs.

Table 13 presents mean ionic and total elemental abundances derived from ORLs and CELs.

WR-PN-Chemistry-Data.1.1

25 Aug 19:03
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Physical and chemical properties of Wolf-Rayet planetary nebulae. Supplementary Data

Table 4 lists observed and dereddened line fluxes on a scale relative to Hb, where Hb = 100.

Table 6 presents electron temperatures and densities derived from CELs.

Table 7 presents electron temperatures derived from He I lines.

Table 8 presents electron temperatures and densities derived from ORLs.

Table 11 presents ionic abundances relative to hydrogen derived from CELs.

Table 12 presents ionic abundances relative to hydrogen derived from ORLs.

Table 13 presents mean ionic and total elemental abundances derived from ORLs and CELs.

WR-PN-Chemistry-Data.1.0

20 Jun 22:00
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Physical and chemical properties of Wolf-Rayet planetary nebulae. Supplementary Data

Table 4 lists observed and dereddened line fluxes on a scale relative to Hb, where Hb = 100.

Table 6 presents electron temperatures and densities derived from CELs.

Table 7 presents electron temperatures derived from He I lines.

Table 8 presents electron temperatures and densities derived from ORLs.

Table 11 presents ionic abundances relative to hydrogen derived from ORLs.

Table 12 presents ionic abundances relative to hydrogen derived from CELs.

Table 13 presents mean ionic and total elemental abundances derived from ORLs and CELs.