Tracing the cold and warm physico-chemical structure of deeply embedded protostars: IRAS 16293−2422 vs. VLA 1623−2417

N. M. Murillo; E. F. van Dishoeck; M. H. D. van der Wiel; J. K. Jørgensen; M. N. Drozdovskaya; H. Calcutt; D. Harsono

doi:10.1051/0004-6361/201731724

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Volume 617 (September 2018)

A&A, 617 (2018) A120

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Table C.1

c-C₃H₂ and C₂H peak intensities.

Molecules	c-C₃ H₂					C₂H

Transition	5–4	9–8	10–9	8_2,6–7_3,5	8_3,6–7_2.5	J = 9/2–7/2 F = 5–4	J = 9/2–7/2 F = 4–3	J = 7/2–5/2 F = 4–3	J = 7/2–5/2 F = 3–2
IRAS 16293−2422 (rms = 10 mJy beam⁻¹)

South^a	240	410	350	90	200	30	30	30	30
Center^a	30	30	30	30	30	170	140	140	110
North^a	30	30	30	30	30	150	130	110	110

VLA 1623−2417 – APEX (rms = 80 mK)

A	...	...	...	...	...	960	616	680	342

Notes. ^(a)For the positions with nondetections, three times the rms noise is used for the calculations.

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