HXHWL 16

0.34 UTI

0.61

C_N

0.35

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 72

Core radius and density 0.6 [pc], 1.8 [pc^-2]

C3 classification AB

C_N 0.61 Moderately populated
C_dens 0.35 Loose
C_C3 0.75 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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HXHWL 16 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 3 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Data

🔍 Search references for HXHWL 16 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–	173.131	-68.095	0.692	-8.82	0.753	1.537
He et al.	2021	173.095	-68.09	0.68	-8.8	0.72	–

💡 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–	1.45	1.39	–	87	0.073	–	–	–
He et al.	2021	1.45	1.39	–	87	0.073	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
LISC 3316	84.7	173.07	-68.08	0.7	-8.82	0.76	1.54	0.01
CWWDL 14104	81.9	173.05	-68.08	0.7	-8.82	0.76	1.54	0.03
Theia 2982	75.0	173.12	-68.1	0.69	-8.82	0.75	1.54	0.01

💡 Note: The % column shows the percentage of members that HXHWL 16 shares with each listed object.

Visualization

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