LP 32

0.01 UTI

0.33

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.03

C_dup

C3 classification DA

Number of members (P>50%) 33

Radius (P>50% members) 1.4 [arcmin]

C_N 0.33 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

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LP 32 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate^* distance, below 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 9 years.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~3.80 kpc) differs significantly from the median photometric distance (~2.73 kpc).

Relatively close Moderate extinction Very young

Data

🔍 Search references for LP 32 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	–	93.715	12.859	0.263	0.924	-1.981	45.64
Loktin & Popova	2017	93.795	12.833	–	1.649	-2.974	–

💡 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
Loktin & Popova	2017	2.73	1.52	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Skiff J0614+12.9	97.0	93.69	12.87	0.27	0.9	-1.98	45.64	0.85

💡 Note: The % column shows the percentage of members that LP 32 shares with each listed object.

Visualization

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