Physical conditions in the gas phases of the giant H II region LMC-N 11 unveiled by Herschel - I. Diffuse [C II] and [O III] emission in LMC-N 11B

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Volume 548 (December 2012)

A&A, 548 (2012) A91

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Table 5

O stars with known spectral types.

Name^a	Type^a	r ^b	f ^c	F([O iii]₈₈)
		(pc)		(× 10^-14 W m^-2)


Eastern half^d		22.6 (20.0)	0.5	24.4
3173 (N11-080)	O7 V	7.2 (6.0)	1.0	1.2
3224^e (N11-050)	O4 V	13.4 (11.2)	0.7	4.7
3204 (N11-048)	O6.5 V	11.0 (9.0)	1.	3.5
3168 (N11-032)	O7 II	12.2 (11.3)	1.	6.2
3223 (N11-013)	O8 V	5.8 (4.1)	1.	0.2
3209^e	O3 III	18.8 (16.2)	0.7	16.6


Western half^d		27.8 (24.5)	0.4	29.3
3061 (N11-031)	ON2 III	18.8 (16.3)	0.3	6.5
3058 (N11-060)	O3 V	17.4 (15.0)	0.3	6.6
3053 (N11-018)	O6 II	17.7 (15.0)	0.3	6.2
3042 (N11-087)	O9.5 V	3.2 (2.2)	0.	0.
3100 (N11-038)	O5 III	10.2 (8.2)	0.5	1.4
3070	O6 V	11.0 (9.0)	0.3	1.3
3126	O6.5 V	10.2 (8.2)	0.7	2.0
3120^e	O5.5 V	12.0 (10.0)	0.7	3.8
3073	O6.5 V	10.2 (8.2)	0.4	1.2
3089	O8 V	6.8 (4.9)	0.5	0.2
3102	O7 V	9.1 (7.0)	0.6	1.0
3103	O9.5 IV	3.4 (2.3)	0.9	0.07
3115	O9 V	4.7 (3.3)	0.9	0.2
3123	O8.5 V	5.8 (4.1)	0.9	0.2

Notes.

^(a)

Spectral type and name are from Parker et al. (1992). The label in parentheses refers to Evans et al. (2006). When available, the spectral type was updated using Evans et al. (2006).

^(b)

Radius of the [O iii]₈₈ emitting sphere containing 99% of the total [O iii]₈₈, assuming an homogenous density of 16 cm^-3. The value between parentheses give the radius of the sphere containing 75% of the total [O iii].

^(c)

Fraction of the [O iii]₈₈ emission falling into the PACS map (assuming a density of 16 cm^-3).

^(d)

The model for each half of N 11B considers all stars located in the same location, it is not a combination of the models from individual stars.

^(e)

Possible composite spectrum in Parker et al. (1992).

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