An infrared and far-UV study of jet-induced star formation in the halo of Centaurus A

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Table 2.

FUV luminosities expected from dust scattering for the northeast and the southwest region of the halo of Cen A.

	$L_{FUV}^{sca}$ $L_{\mathrm{FUV}}^{\mathrm{sca}}$ [erg/s]		$L_{FUV}^{obs}$ $L_{\mathrm{FUV}}^{\mathrm{obs}}$ [erg/s]

Power-law index q^(a)	−3.5	−4.5
Northeast	(1.9 ± 0.4)×10³⁹	(0.6 ± 0.1)×10³⁹	(11.0 ± 0.1)×10³⁹
Southwest	(6.6 ± 1.2)×10³⁹	(2.2 ± 0.4)×10³⁹	(1.9 ± 0.1)×10³⁹

Notes.

^(a)

Dust size distribution n(a) is proportional to a^q (Mathis et al. 1977).

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