Resolved molecular gas and star formation in massive unquenched spirals - I. UGC 8179

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Table 3.

Properties computed by SED fitting.

	SFR₁₀₀	SFR₁₀	log₁₀M_★	χ_red²
	M_⊙ yr⁻¹	M_⊙ yr⁻¹	log₁₀(M_⊙)
4 R_e	15.58 ± 4.57	10.29 ± 6.26	11.62 ± 0.06	0.15
PB_CO	9.34 ± 2.26	4.76 ± 3.52	11.54 ± 0.06	0.24

	${log}_{10} τ_{dep}^{100}$ $Mathematical equation: $ \log_{10}\tau_{\mathrm{dep}}^{100} $$	${log}_{10} τ_{dep}^{10}$ $Mathematical equation: $ \log_{10}\tau_{\mathrm{dep}}^{10} $$	log₁₀f_mol

4 R_e	≥8.82 ± 0.13	≥9.00 ± 0.31	≥ − 1.61 ± 0.06
PB_CO	9.04 ± 0.11	9.33 ± 0.41	−1.53 ± 0.07

Notes. These results were obtained after flux extraction on the convolved maps (see Section 3.2) in an ellipse of semimajor axis a = 4 R_e and in the region of the primary beam at NOEMA’s HPBW (see Fig. 2).

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