Gas-phase Fe/O and Fe/N abundances in star-forming regions - Relations between nucleosynthesis, metallicity, and dust

Home

All issues

Volume 690 (October 2024)

A&A, 690 (2024) A248

Full HTML

Open Access

Table 1

Ionic and total Fe abundances compared to the predictions of the Fe-ICFs from Rodríguez & Rubin (2005) and Izotov et al. (2006), which are derived from photoionization models.

Ref.	Region	Fe+/H+	Fe²⁺/H⁺	Fe³⁺/H⁺	Fe⁴⁺/H⁺	Ionic Sum	ICF	ICF
							R&R05^(𝑔)	I06^(h)
t² = 0
D83	HS1851+6933^(a)	–	${5.20}_{- 0.05}^{+ 0.06}$ $5.20_{ - 0.05}^{ + 0.06}$	5.59 ± 0.04	${4.49}_{- 0.04}^{+ 0.05}$ $4.49_{ - 0.04}^{ + 0.05}$	5.76 ± 0.03	5.88 ± 0.06	${6.12}_{- 0.05}^{+ 0.06}$ $6.12_{ - 0.05}^{ + 0.06}$
D451	W1702+18^(a)	–	${4.95}_{- 0.03}^{+ 0.04}$ $4.95_{ - 0.03}^{ + 0.04}$	${5.28}_{- 0.05}^{+ 0.06}$ $5.28_{ - 0.05}^{ + 0.06}$	4.53 ± 0.05	5.50 ± 0.04	5.81 ± 0.03	6.07 ± 0.03
D224	Orion Nebula^(b)	${4.69}_{- 0.05}^{+ 0.04}$ $4.69_{ - 0.05}^{ + 0.04}$	5.55 ± 0.03	5.71 ± 0.07	–	5.96 ± 0.04	6.11 ± 0.03	6.32 ± 0.03
D235	NGC2579^(c)	–	5.40 ± 0.03	${5.24}_{- 0.14}^{+ 0.16}$ $5.24_{ - 0.14}^{ + 0.16}$	–	${5.63}_{- 0.07}^{+ 0.06}$ $5.63_{ - 0.07}^{ + 0.06}$	5.88 ± 0.03	6.11 ± 0.03
D236	NGC3576^(d)	4.59 ± 0.06	${5.53}_{- 0.03}^{+ 0.04}$ ${5.53_{ - 0.03}^{ + 0.04}}$	${5.72}_{- 0.08}^{+ 0.09}$ ${5.72_{ - 0.08}^{ + 0.09}}$	–	5.95 ± 0.05	5.95 ± 0.03	${6.18}_{- 0.03}^{+ 0.04}$ $6.18_{ - 0.03}^{ + 0.04}$
D283	Mrk71 ^(e)	–	${4.32}_{- 0.10}^{+ 0.18}$ ${4.32_{ - 0.10}^{ + 0.18}}$	${4.97}_{- 0.07}^{+ 0.08}$ ${4.97_{ - 0.07}^{ + 0.08}}$	–	5.06 ± 0.06	5.45 ± 0.14	${5.72}_{- 0.10}^{+ 0.18}$ $5.72_{ - 0.18}^{ + 0.18}$
D403	SMC-N88A^(f)	–	${4.99}_{- 0.03}^{+ 0.04}$ $4.99_{ - 0.03}^{ + 0.04}$	5.47 ± 0.04	–	5.59 ± 0.03	${6.00}_{- 0.06}^{+ 0.08}$ $6.00_{ - 0.06}^{ + 0.08}$	${6.27}_{- 0.03}^{+ 0.04}$ $6.27_{ - 0.03}^{ + 0.04}$
t² > 0
D83	HS1851+6933^(a)	–	${5.20}_{- 0.05}^{+ 0.07}$ $5.20_{ - 0.05}^{ + 0.07}$	${6.48}_{- 0.09}^{+ 0.13}$ $6.48_{ - 0.09}^{ + 0.13}$	${5.05}_{- 0.06}^{+ 0.09}$ $5.05_{ - 0.06}^{ + 0.09}$	${6.52}_{- 0.10}^{+ 0.11}$ $6.52_{ - 0.10}^{ + 0.11}$	6.29 ± 0.06	${6.58}_{- 0.05}^{+ 0.06}$ $6.58_{ - 0.05}^{ + 0.06}$
D451	W1702+18^(a)	–	4.94 ± 0.03	${5.63}_{- 0.05}^{+ 0.07}$ $5.63_{ - 0.05}^{ + 0.07}$	${4.74}_{- 0.04}^{+ 0.05}$ $4.74_{ - 0.04}^{ + 0.05}$	${5.76}_{- 0.04}^{+ 0.05}$ $5.76_{ - 0.04}^{ + 0.05}$	5.98 ± 0.03	6.25 ± 0.03
D224	Orion Nebula^(b)	${4.69}_{- 0.04}^{+ 0.05}$ $4.69_{ - 0.04}^{ + 0.05}$	5.55 ± 0.03	${5.75}_{- 0.09}^{+ 0.10}$ $5.75_{ - 0.09}^{ + 0.10}$	–	5.99 ± 0.05	6.12 ± 0.03	6.34 ± 0.03
D235	NGC2579^(c)	–	5.40 ± 0.03	5.84 ± 0.14	–	5.97 ± 0.10	6.10 ± 0.03	6.31 ± 0.03
D236	NGC3576^(d)	4.59 ± 0.05	${5.53}_{- 0.03}^{+ 0.04}$ ${5.53_{ - 0.03}^{ + 0.04}}$	${6.42}_{- 0.09}^{+ 0.13}$ ${6.42_{ - 0.09}^{ + 0.13}}$	–	6.48 ± 0.09	6.19 ± 0.04	6.40 ± 0.03
D283	Mrk71 ^(e)	–	${4.33}_{- 0.11}^{+ 0.17}$ ${4.33_{ - 0.11}^{ + 0.17}}$	${5.49}_{- 0.17}^{+ 0.47}$ ${5.49_{ - 0.17}^{ + 0.47}}$	–	${5.51}_{- 0.29}^{+ 0.31}$ $5.51_{ - 0.29}^{ + 0.31}$	5.70 ± 0.14	${6.03}_{- 0.11}^{+ 0.19}$ $6.03_{ - 0.11}^{ + 0.19}$
D403	SMC-N88A^(f)	–	${4.99}_{- 0.03}^{+ 0.04}$ ${4.99_{ - 0.03}^{ + 0.04}}$	${5.78}_{- 0.06}^{+ 0.09}$ ${5.78_{ - 0.06}^{ + 0.09}}$	–	${5.84}_{- 0.06}^{+ 0.07}$ $5.84_{ - 0.06}^{ + 0.07}$	6.16 ± 0.04	${6.44}_{- 0.03}^{+ 0.04}$ $6.44_{ - 0.03}^{ + 0.04}$

Notes. These values were calculated both considering a homogeneous nebular temperature (t² = 0) and considering the effect of t² > 0. The abundance values are presented in units of 12+log(X/H). The reference number is also shown for consistency with the values in Table D2. ^(a)Izotov et al. (2021); ^(b)Méndez-Delgado et al. (2021a); ^(c)Esteban et al. (2013); ^(d)García-Rojas et al. (2004);^(e)Esteban et al. (2009); ^(f)Domínguez-Guzmán et al. (2022); ^(𝑔)Rodríguez & Rubin (2005); ^(h)Izotov et al. (2006).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.