The nature of the interstellar medium of the starburst low-metallicity galaxy Haro 11: a multi-phase model of the infrared emission

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Table 1

General properties of Haro 11.

Quantity	Value	Reference

RA (J2000)	00h36′52.5″	NED^a
Dec (J2000)	−33°33′19″	NED
Distance	84 Mpc	NED^b
12+log(O/H)	8.2	Guseva et al. (2012)
Optical size	0.4′×0.5′	NED
L _TIR ^c	1.4×10¹¹ L_⊙	Galametz et al. (2009)
L _FUV	2×10¹⁰ L_⊙	Grimes et al. (2007)
L _X−rays	4.4×10⁷ L_⊙	Grimes et al. (2007)
L _Lyα	1.9×10⁸ L_⊙	Hayes et al. (2007)
L _Hα	8×10⁸ L_⊙	Östlin et al. (1999)

Notes. All luminosities are scaled to the distance chosen in this paper of 84 Mpc.

^(a)

NASA/IPAC Extragalactic Database.

^(b)

This distance is derived with a Hubble constant H₀ = 73 km s^-1 Mpc^-1.

^(c)

L_TIR is the integrated SED from 3 to 1100 μm.

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