Pismis 14

(MWSC 1678; OCL 780; ESO 166 16)

0.18 UTI

0.0

C_N

0.03

C_dens

0.12

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 12

Radius (P>50% members) 7.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.12 Very low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

Pismis 14 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.25 kpc) differs significantly from the median photometric distance (~1.77 kpc).

⚠️ 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 Low mass Intermediate age

Data

🔍 Search references for Pismis 14 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	142.458	-52.797	0.235	-4.545	2.728	61.818
Just et al.	2023	142.465	-52.777	–	–	–	–
Bica et al.	2019	142.456	-52.773	–	–	–	–
Kharchenko et al.	2016	142.465	-52.777	–	–	–	–
Dias et al.	2014	142.463	-52.783	–	-3.77	4.83	–
Kharchenko et al.	2013	142.47	-52.78	–	-6.65	4.71	–
Dias et al.	2002	142.463	-52.783	–	-3.69	4.79	–

💡 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]	Bfr	BSS
Just et al.	2023	–	–	–	226	–	44	–	–
Kharchenko et al.	2016	1.77	1.48	–	226	–	–	–	–
Kharchenko et al.	2013	1.77	1.48	–	226	–	–	–	–
Dias et al.	2002	1.31	1.74	–	22	–	–	–	–

Visualization

ℹ️