NS14

(AFGL5216; BIP14; IRAS 06567-0355; MWSC 1047)

0.16 UTI

0.0

C_N

0.03

C_dens

0.12

C_C3

0.31

C_lit

1.0

C_dup

N_m (P>50%) 15

Core radius and density 3.5 [pc], 0.1 [pc^-2]

C3 classification CD

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.12 Very low quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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NS14 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Young

Bica et al. (2003)
Classified as infrared cluster (IRC).

Lada & Lada (2003)
Embedded cluster within ∼2 Kpc of the Sun.

Data

🔍 Search references for NS14 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	104.837	-4.003	0.391	0.29	4.031	72.516
Just et al.	2023	104.813	-3.969	–	–	–	–
Dib et al.	2018	104.82	-3.97	–	–	–	–
Joshi et al.	2016	123.78	-4.075	–	–	–	–
Kharchenko et al.	2016	104.813	-3.969	–	–	–	–
Kharchenko et al.	2013	104.82	-3.97	–	0.41	4.36	39.6
Lada & Lada	2003	104.816	-3.994	–	–	–	–
Bica et al.	2003	104.815	-3.986	–	–	–	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	B_frac	BSS
UCC	99999–	1.94	2.03	–	22	–	142	–	–
Just et al.	2023	–	–	–	22	–	224	–	–
Dib et al.	2018	1.94	–	–	22	–	–	–	–
Joshi et al.	2016	1.61	1.64	–	124	–	–	–	–
Kharchenko et al.	2016	1.94	2.03	–	22	–	–	–	–
Kharchenko et al.	2013	1.94	2.03	–	22	–	–	–	–
Lada & Lada	2003	1.40	–	–	–	–	61	–	–

Visualization

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