Identification and characterization of nascent planetary nebulae with OH and H2O masers

Open Access

Table B.3

OH maser emission in our ATCA and VLA observations of IRAS 17487–1922

Maser coordinates		δ_R.A.	δ_dec	Transition	V_LSR	S_ν
R.A.(J2000)	Dec(J2000)	(arcsec)	(arcsec)	(MHz)	(km s⁻¹)	(Jy)
17:51:44.89120	−19:23:46.8	0.0020	0.4	1612	−39.18	0.39±0.07
17:51:44.79420	−19:23:46.66	0.0013	0.20	1612	−39.00	0.41±0.04
17:51:44.9810	−19:23:41.91	0.015	0.24	1612	−38.82	0.44±0.05
17:51:44.91960	−19:23:40.9	0.0019	0.4	1612	−38.64	0.44±0.09
17:51:44.8501	−19:23:46.8	0.004	0.6	1612	−38.37	0.345±0.011
17:51:44.98140	−19:23:40.21	0.0020	0.31	1612	−38.10	0.44±0.07
17:51:45.12	−19:23:42.9	0.4	0.4	1612	−38.15	0.58±0.05
17:51:44.711	−19:23:43.41	0.21	0.21	1612	−39.06	0.48±0.08
17:41:45.36	−19:23:42.0	0.3	0.4	1612	−39.60	0.38±0.04

Notes. The VLA observations are marked with the frequency of the transition in boldface. The ones with normal fonts, represent the ATCA observations

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