A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) - XII. Ionised gas emission in the inner regions of lenticular galaxies

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Table 8.

Dust masses.

NGC	M_dust(SED)	M_dust(A(g))	G/D ^(b)

Units	M_⊙	M_⊙
4262	−	−	−
4429	1.83 × 10⁶ ± 2.9 × 10⁵	5.0 × 10⁴	86.1 (226.4)
4459	1.50 × 10⁶ ± 1.1 × 10⁵	2.4 × 10⁴	90.5 (318.4)
4469 ^(a)	7.67 × 10⁶ ± 3.8 × 10⁵	2.0 × 10⁴	−
4476	1.06 × 10⁶ ± 1.4 × 10⁵	5.7 × 10³	67.1 (138.1)
4477	5.81 × 10⁵ ± 1.3 × 10⁵	4.0 × 10⁴	30.9
4526	9.95 × 10⁶ ± 1.6 × 10⁶	9.4 × 10⁴	40.8 (31.6)
4552	6.02 × 10⁶ ± 3.8 × 10⁶	−	−

Notes.

^(a)

A(g) measured only within the star-forming disc, thus the dust mass coming from A(g) is a lower limit because filaments of dust are seen outside the selected region.

^(b)

Gas-to-dust ratio measured using dust masses derived from the SED fitting analysis and molecular gas masses with CARMA (and ALMA) data.

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