A morpho-kinematic and spectroscopic study of the bipolar nebulae: M 2−9, Mz 3, and Hen 2−104

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Table A.4

2MASS NIR (HJKs) colours of various PNe.

Object	Type	H	J	Ks

NGC 1535	PN	12.539	12.647	12.577
NGC 2438	PN	12.672	12.526	12.509
NGC 2440	PN	15.671	15.037	15.203
NGC 3132	PN	9.754	9.731	9.723
NGC 3242	PN	12.102	12.461	11.748
NGC 6302	PN	11.255	11.706	9.442
NGC 7009^†	PN	9.325	9.456	8.748
NGC 7027	PN	9.613	8.37	7.443
NGC 2392	PN	10.872	10.919	10.936
MyCn 18	PN	11.554	11.603	10.808
Mz 3^†	PN	9.352	7.355	5.608
PB 5	PN	12.488	11.897	10.625
PB 3	PN	13.899	13.703	12.651
He 2-36	PN	9.867	9.623	9.463
He 2-39	PN	13.474	12.614	12.338
He 2-63	PN	15.55	15.427	14.613
He 2-67	PN	13.43	13.431	12.454
He 2-70	PN	12.544	11.497	11.180
He 2-84	PN	14.527	13.422	13.077
He 2-85	PN	15.198	14.305	13.681
He 2-86	PN	12.155	11.853	10.789
He 2-96	PN	12.577	12.228	11.178
My 60^††	PN	12.604	12.379	11.635
Pe 1-1	PN	12.457	12.065	10.931
ESO 095-1	PN	15.201	13.798	11.867
ESO 320-2	PN	15.166	14.157	13.606
BMP J1128-6121	PN	14.155	13.478	12.340
NGC 3918	PN	11.691	11.568	10.422
K 1-23	PN	16.701	15.941	16.584
Wray 16-128	PN	15.761	15.078	14.872
MaC 1-2	PN	13.713	13.446	13.315
He 2-102	PN	14.636	14.31	13.661
He 2-103	PN	14.971	14.34	13.612
He 2-108	PN	12.173	12.103	11.877
He 2-109	PN	16.338	15.832	15.061^a
He 2-115	PN	12.033	11.724	10.598
He 2-117	PN	11.811^a	11.424^a	10.195^a
He 2-133	PN	12.132	11.72	10.579
NGC 5939	PN	14.777	13.782	12.700^a
NGC 6326	PN	14.747	14.939	14.104
StWr 4-10	PN	14.335	14.209	13.824
M 2-9^†	PN	11.198	9.177	6.996
M 1-91	PN	14.099	11.841	9.710
K 3-31	PN	13.806	13.339	12.300
K 3-56	PN	15.973	14.895^a	14.689
K 3-87	PN	16.214	15.684	14.919
K 4-41	PN	15.602^a	13.796^a	14.473
M 2-50	PN	15.333	15.242	14.456
Bl 2-1	PN	13.473	12.607	11.16
Hen 2-440	PN	13.603	12.686	12.414
NGC 6807	PN	12.753	12.826	12.069
M 1-69	PN	13.261	13.207	12.286
IC 4846	PN	12.681	12.835	11.897
K 4-8	PN	14.792	14.802	13.946
Sa 2-237	PN	13.065	12.566	11.817
MaC 1-11	PN	14.179	13.779	13.107

Notes. The data have been obtained from the 2MASS All-Sky Catalog of Point Sources (Cutri et al. 2003b).

^(†)

Objects of interest within this paper.

^(††)

From Skrutskie et al. (2006).

^(a)

Uncertain value.

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