Multiwavelength study of the HII region LHA 120-N11 in the Large Magellanic Cloud with eROSITA

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Volume 686 (June 2024)

A&A, 686 (2024) A307

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Table 3

Total energy of hot plasma and stellar energy input.

Region	E_p [10⁵¹] f^0.5 erg	Number of high-mass stars^(†)	Number of SNe	E_stellar[10⁵¹] erg^(††)	E_HI[10⁵¹] erg	Energy balance
Dark lane	${1.26}_{- 0.31}^{+ 0.73}$ $1.26_{ - 0.31}^{ + 0.73}$	4	0–1	1.3–3.6	~5	E_stellar ~ E_p < E_HI
Bubble	${1.42}_{- 0.13}^{+ 0.21}$ $1.42_{ - 0.13}^{ + 0.21}$	28	1–3	5.8–10.0	~4	E_stellar ~ E_p + E_HI
Small	${0.72}_{- 0.26}^{+ 0.33}$ $0.72_{ - 0.26}^{ + 0.33}$	2	0–1	0.6–1.8	~2	E_stellar ~ E_p ~ E_HI
Diffuse	${1.63}_{- 0.10}^{+ 0.11}$ $1.63_{ - 0.10}^{ + 0.11}$	0	0–1	1.3–3.6	~2	E_stellar ~ E_p ~ E_HI

Notes. ^(†)References of the Bubble region and the other regions are Mokiem et al. (2007) and Bonanos et al. (2009), respectively.^(††)E_stellar included the energy input of the SNae and the previous star formation.

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