Detections of Long Carbon Chains CH 3 CCCCH, C 6 H, linear -C 6 H 2 and C 7 H in the Low-Mass Star Forming Region L1527

M. Araki, S. Takano, N. Sakai, S. Yamamoto, T. Oyama, N. Kuze, K. Tsukiyama
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Abstract

the two states. In the present observations, the Ka = 0 line of para species of l-C6H2 was detected, although the detection was limited for the Ka = 1 line of ortho species so far except for IRC+10216. The column densities of the ortho and para species of l-C6H2 were independently obtained to be 1.3 × 10 11 and 0.6 × 10 11 cm −2 , respectively. C7H was detected for the first time except for IRC+10216. The column density of C7H was estimated to be 6.2 × 10 10 cm −2 from the J = 24.5‒23.5 and 25.5‒24.5 lines. These results of detections would
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低质量恒星形成区L1527中长碳链ch3 CCCCH、c6h、线性c6h2和c7h的检测
两个州。在本观察中,检测到l-C6H2对种的Ka = 0系,但目前除IRC+10216外,对种的Ka = 1系检测有限。l-C6H2的邻位和对位柱密度分别为1.3 × 10 11和0.6 × 10 11 cm−2。除IRC+10216外,C7H为首次检出。从J = 24.5-23.5和25.5-24.5谱线估计C7H柱密度为6.2 × 10 10 cm−2。这些检测结果将
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