Fig. 7
Abundances of cyanopolynes in different sources: IRAS 16293 outer envelope (IT20) and inner region (Iin; this work), cold clouds (CC; Winstanley & Nejad 1996; Miettinen 2014), comet Hale-Bopp at 1 AU assuming H2O/H2 = 5 × 10-5 (Comets; Bockelé- Morvan et al. 2000), first hydrostatic core sources (FHSC; Cordiner et al. 2012), warm carbon-chain chemistry sources (WCCC; Sakai et al. 2008, 2004), massive hot cores (HC; Schöier et al. 2002; Esplugues et al. 2013), outflow sources (OF; Bachiller & Pérez Gutiérrez 1997; Schöier et al. 2002, Galactic Centre clouds (GCC; Marr et al. 1993; Aladro et al. 2011), and external galaxies (EG; Aladro et al. 2011).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.