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

Open Access

Table E.1

List of all confirmed water fountains.

Name	Alt. name	V_range^a km s⁻¹	Reference^b
IRAS 15103–5754	GLMP 405	70	1
IRAS 15445–5449	OH 326.5–0.4	90	2
IRAS 16342–3814	OH 344.1+5.8	260	3
IRAS 16552–3050	GLMP 498	170	4
IRAS 17291–2147	GLMP 498	70	5
IRAS 18019–2216	SCHB 281	20	This work
IRAS 18043–2116	OH 9.1–0.4	800	6, 7
IRAS 18113–2503	PM 1–221	500	8
IRAS 18139–1816	OH 12.8–0.9	50	9
IRAS 18286–0959	OH 21.80–0.13	200	10
IRAS 18443–0231	RFS 505	80	This work
IRAS 18450–0148	W43A	180	11
IRAS 18455+0448		40	12
IRAS 18460–0151	OH 31.0–0.2	310	13
IRAS 18464–0140	OH 31.21–0.18	30	This work
IRAS 18596+0315	OH 37.1–0.8	60	5
IRAS 19134+2131		100	14
IRAS 19190+1102	PM 1–298	100	15

Notes.^a Velocity range of the H₂O masers to date.^b Interferometric confirmation as WF and velocity range: 1. Gómez et al. (2015b). 2. Pérez-Sánchez et al. (2011). 3. Claussen et al. (2009). 4. Suárez et al. (2008). 5. Gómez et al. (2017). 6. Walsh et al. (2009) 7. Uscanga et al. (2023). 8. Gómez et al. (2011). 9. Boboltz & Marvel (2005). 10. Yung et al. (2011). 11. Imai et al. (2002). 12. Vlemmings et al. (2014). 13. Imai et al. (2013). 14. Imai et al. (2004). 15. Day et al. (2010).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.