HXWHB 14

0.53 UTI

0.64

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 78

Stellar density (N₅₀/rad) 17.7 [N/pc²]

C3 classification AA

C_N 0.64 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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HXWHB 14 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high 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 6 years.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Very young

Data

🔍 Search references for HXWHB 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–	302.379	38.29	0.277	-2.599	-4.876	–
Hao et al.	2020	302.38	38.29	0.27	-2.61	-4.89	–

💡 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–	3.67	3.19	–	9	–	–	–	–
Hao et al.	2020	3.67	3.19	–	9	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 372	93.6	302.38	38.29	0.27	-2.58	-4.87	–	0.1

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

Visualization

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