Kinematic study of planetary nebulae in NGC 6822 | Astronomy & Astrophysics (A&A)

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Table 2

PNe, H ii regions, and stars analyzed in NGC 6822.

Object ID^a	RA (J2000)	Dec (2000)	Other ID

PN2^b	19:45:56.6	−14:40:53.4	PN5^d
PN4^b^c	19:45:01.4	–14:41:33.0	S30^e PN4^d
PN6^b^c	19:44:00.7	–14:42:43.6	PN1^d
PN7^c	19:44:49.1	−14:43:00.6	PN2^d
PN8^b	19:42:02.2	−14:43:42.2	PN6^d
PN10^c	19:45:22.0	−14:43:28.0	PN19^d
PN12^c	19:44:58.8	−14:44:45.0	S14^e, PN14^d
PN14^b^c	19:45:07.5	–14:47:35.8	S33^e ,PN7^d
PN16^c	19:44:58.6	−14:46:10.0	S16^e, PN13^d
PN20^b	19:45:11.5	−14:48:53.6	PN20^f

H V^g	19:44:52.4	−14:43:13.4	–
H X^g	19:45:5.23	−14:43:16.7	–
H ii 18^c	19:44:42.6	–14:50:30.2	H ii 18^d, S10^e
H ii 15^c	19:44:57.2	–14:47:50.6	H ii 08^d, S28^e
A 13^h	19:44:53.4	−14:46:42	A supergiant
A 101^h	19:44:56.5	−14:46:14	A supergiant

Notes.

^(a)

Names as in Hernández-Martínez & Peña (2009), except for H V and H X.

^(b)

Observed at LCO with MIKE.

^(c)

Observed at SPM with MES.

^(d)

Leisy et al. (2005).

^(e)

Killen & Dufour (1982).

^(f)

Richer & McCall (2007).

^(g)

Hubble (1925).

^(h)

Venn et al. (2001).

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