Dense gas and star formation in the outer Milky Way

Open Access

Fig. 14

Link between dense gas mass (HCN or HCO⁺ luminosity on the x-axis) and SF rate (IR luminosity on the y-axis). The line shows a linear relation with . HCN data are shown as filled triangles and HCO⁺ as open squares. The outer disk data presented in this paper are shown in blue. The sources for the data are: Chin et al. (1997, 1998), Gao & Solomon (2004b), Gao et al. (2007), Brouillet et al. (2005), Wu et al. (2005), Ma et al. (2013), Buchbender (2014), Krips et al. (2008), Juneau et al. (2009), Privon et al. (2015), Graciá-Carpio et al. (2008), García-Burillo et al. (2012), Chen et al. (2015, 2017), Usero et al. (2015).

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