BPI 14

0.20 UTI

0.68

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.42

C_dup

N₅₀ (P>50% members) 86

Stellar density (N₅₀/rad) 9.1 [N/pc²]

C3 classification AB

C_N 0.68 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.42 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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BPI 14 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 14 years.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close Moderate extinction Very young

Data

🔍 Search references for BPI 14 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–	82.085	34.411	0.455	0.219	-2.311	25.032
Camargo et al.	2012	82.25	34.4	–	–	–	–

💡 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–	2.7	1.98	–	2	–	–	–	–
Camargo et al.	2012	2.70	1.98	–	2	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Stock 8	58.1	81.96	34.43	0.46	0.08	-2.34	-59.37	0.91
CBB 5	36.0	82.05	34.45	0.46	0.14	-2.09	11.91	0.16
HSC 1356	1.2	81.86	34.39	0.46	0.17	-1.87	79.39	0.08

💡 Note: The % column shows the percentage of members that BPI 14 shares with each listed object.

Visualization

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