Doubly substituted isotopologues of HCCCN in TMC-1: Detection of D13CCCN, DC13CCN, DCC13CN, DCCC15N, H13C13CCN, H13CC13CN, HC13C13CN, HCC13C15N, and HC13CC15N

Open Access

Fig. 1.

Observed lines of D¹³CCCN, DC¹³CCN, DCC¹³CN, and DCCC¹⁵N towards TMC-1 (CP) with the Yebes 40 m telescope (histogram black spectra). The red curves present the synthetic spectra obtained using LVG approximation (see Sect. 3.1 and Table A.5). The dashed line represents the 3σ level.

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