History of the solar-type protostar IRAS 16293–2422 as told by the cyanopolyynes

A. Jaber Al-Edhari; C. Ceccarelli; C. Kahane; S. Viti; N. Balucani; E. Caux; A. Faure; B. Lefloch; F. Lique; E. Mendoza; D. Quenard; L. Wiesenfeld

doi:10.1051/0004-6361/201629506

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Volume 597 (January 2017)

A&A, 597 (2017) A40

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Fig. 4

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Results of the HC₃N modelling. The best reduced χ² optimised with respect to X_in and X_out as a function of T_jump.

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