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J/A+A/663/A177
  High-mass star-forming regions cyanopolyyne (Wang+, 2022)
img(gal)
    J/A+A/663/A177/table2Far infrared properties of our HC3N sources (21 rows)
    J/A+A/663/A177/tableb1(c)The HC3N (J = 2-1) transitions detected with the TMRT (41 rows)
    J/A+A/663/A177/tableb2(c)The HC5N (J=3-2) and HC7N (J=15-14) transitions detected with TMRT (12 rows)
    J/A+A/663/A177/tableb3(c)The column density and the relative abundance for HC3N, HC5N, and HC7N. (38 rows)
    J/A+A/663/A177/tableb4The integrated line intensities of other molecules (23 rows)
    J/A+A/663/A177/tablec1(c)Sources without HC3N (J=2-1) detection (85 rows)

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       (c)  indicates tables which contain celestial coordinates 
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