(Sub)millimeter emission lines of molecules in born-again stars

D. Tafoya; J. A. Toalá; W. H. T. Vlemmings; M. A. Guerrero; E. De Beck; M. González; S. Kimeswenger; A. A. Zijlstra; Á. Sánchez-Monge; S. P. Treviño-Morales

doi:10.1051/0004-6361/201630074

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Volume 600 (April 2017)

A&A, 600 (2017) A23

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Table 3

Noise characteristics for non-detected molecular transitions.

Molecule	Transition	Rest frequency	rms^a
		(GHz)	(mJy)

V4334 Sgr

CO	J = 3 → 2	345.79599	57
CO	J = 2 → 1	230.53800	68
CO	J = 1 → 0	115.27120	13
¹³CO	J = 1 → 0	110.20135	6

V605 Aql

H¹³CN	J = 4 → 3	345.33976	29
¹³CO	J = 3 → 2	330.58797	86

A30

CO	J = 2 → 1	230.53800	24
CO	J = 1 → 0	115.27120	16
¹³CO	J = 1 → 0	110.20135	9
HCN	J = 1 → 0	88.63185	7

A78

CO	J = 1 → 0	115.27120	10
¹³CO	J = 1 → 0	110.20135	6
HCN	J = 1 → 0	88.63185	6

Notes.

^(a)

Channel-to-channel 1σ rms noise of the spectrum smoothed to a velocity resolution of 20 km s^-1.

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