Clustered star formation at early evolutionary stages - Physical and chemical analysis of the young star-forming regions ISOSS J22478+6357 and ISOSS J23053+5953

Open Access

Fig. 9

HOG results for ISOSS J22478+6357 (top panel) and ISOSS J23053+5953 (bottom panel). The peak projected Rayleigh statistic V is shown for each transition pair (Sect. 4.2.2). Examples of high spatial correlations in velocity space are shown in Fig. 10.

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