A search for the OH 6035 MHz line in high-mass star-forming regions

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Table 2

Variability indices of 6035 MHz emission for the main feature on timescales of 2 (vi₂), 10 (vi₁₀), and 25 (vi₂₅) years.

Source	vi₂	vi₁₀	vi₂₅
G10.320−00.259	0.04	0.02
G10.958+00.022	0.02	0.12
G11.034+00.062	0.04	0.03	0.79
G11.904−00.141	0.30	0.78	0.78
G12.209−00.102	0.72
G12.681−00.182	0.42	0.73
G15.035−00.677^(1),(2)	0.06	0.40	0.48
G20.237+00.065	0.30	0.24	0.35
G24.148−00.009	0.34	0.54
G25.650+01.049	0.03	0.09
G25.710+00.044	0.21
G28.146−00.005	0.25
G28.201−00.049		0.31	0.34
G30.771−00.804		0.08
G34.257+00.153^(3),(2)		0.46	0.70
G34.267−00.210	0.02
G35.025+00.350	0.18	0.26	0.44
G43.149+00.013	0.12	0.16	0.44
G45.467+00.053⁽⁴⁾	0.02	0.10	0.20
G48.990−00.299	0.16	0.20
G49.490−00.388^(5),(2)	0.02	0.24	0.67
G80.861+00.383	0.39
G81.871+00.781⁽⁶⁾	0.18
G85.410+00.003	0.17
G108.766−00.986	0.22
G111.542+00.777	0.28
G133.947+01.064⁽⁷⁾	0.11
G183.348−00.575	0.53

Notes. For sources with complex spectra, the velocity and polarisation of the feature used are noted. New detections are in bold. ⁽¹⁾ 21.5 km s⁻¹ LHC; ⁽²⁾large changes in the spectrum shape; ⁽³⁾ 58.4 km s⁻¹ RHC; ⁽⁴⁾ 66.38 km s⁻¹ LHC; ⁽⁵⁾ 55.0 km s⁻¹ RHC; ⁽⁶⁾ 7.87 km s⁻¹ RHC; ⁽⁷⁾ –43.3 km s⁻¹ LHC.

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