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Detection of Aliphatically Deuterated Aromatic Hydrocarbons in the Large Magellanic Cloud 30 Doradus Star-forming Complex

  • Authors: Junhao Peng, Xuejuan Yang, Aigen Li

Junhao Peng et al 2026 The Astrophysical Journal 1010 .

  • Provider: AAS Journals

Caption: Figure 8.

Left panel (a): relation between the 3.4 μm aliphatic C–H stretch and the 6.85 μm aliphatic C–H deformation. Right panel (b): I3.4/I3.3 versus I6.85/I6.2. The results for R3 are indicated by the dashed open circle due to its low-quality spectrum, and this region has been excluded from the correlation analysis. While I3.4 is not correlated with I6.85, I3.4/I3.3 is positively correlated with I6.85/I6.2, confirming the aliphatic nature of the 6.85 μm band. That the 3.4 μm emitter and the 6.85 μm emitter are different in size explains why I3.4 is not correlated with I6.85.

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