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Table 2

ALMA molecular line observations details.

Name Spectral lines(a) ν(b) (GHz) Reference(c)
B335 C2H (JN‚F = 7/2з,4−5/22,з) 262.004260 Imai et al. (2016)
C2H (JN‚F = 7/23,3−5/22,2) 262.006482
CS (J = 5−4) 244.935644
c-C3H2 (52‚3−43‚2) 249.054368

L1448 IRS2 C2H (JN‚F = 5/2з‚з−3/22,2) 262.064986 Zhang et al. (in prep.)
C2H (JN‚F = 5/2з‚2−3/22,1) 262.067469
CS (J = 5−4) 244.935644

NGC1333 IRAS4A C2H (JN‚F = 7/2з,4−5/22,3) 262.004260 Chuang et al. (2021)
C2H (JN‚F = 7/2з,з−5/22,2) 262.006482
CS (J = 5−4) 244.935644
SO(NJ = 7(6)−6(5)) 261.843684

Serpens Emb 8 C2H (JN‚F = 7/2з,4−5/22,з) 262.004260 van Gelder et al. (2020)
C2H (JN‚F = 7/2з,з−5/22,2) 262.006482
SO(NJ = 7(6)−6(5)) 261.843684
Serpens Emb 8(N) C2H (JN‚F = 7/2з,4−5/22,з) 262.004260 Le Gouellec et al. (2019)
C2H (JN‚F = 7/2з,з−5/22,2) 262.006482
SO(NJ = 6(5)−5(4)) 219.949433 Tychoniec et al. (in prep.)

Notes. For the CCH spectral lines presented in the figures below, we integrated over the two hyperfine structures in order to construct the moment 0 maps. (a) Spectral lines that we present in this study. (b) Frequency of spectral line observations. (c) Reference of the publication(s) presenting the ALMA molecular line dataset(s).

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