LP 34

0.28 UTI

0.26

C_N

0.78

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 26

Radius (P>50% members) 9.1 [arcmin]

C_N 0.26 Poorly populated
C_dens 0.78 Dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

ℹ️

LP 34 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a close^* distance, above 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.

(*): The parallax distance estimate (~0.98 kpc) differs significantly from the median photometric distance (~3.53 kpc).

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

Distant Moderate extinction Very young

Data

🔍 Search references for LP 34 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	95.308	18.828	1.024	-1.812	-2.853	-10.302
Loktin & Popova	2017	95.28	18.807	–	2.106	-5.854	–

💡 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	3.53	1.10	–	4	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 10	80.8	95.29	18.84	1.01	-1.8	-2.85	-10.86	0.07

💡 Note: The % column shows the percentage of members that LP 34 shares with each listed object.

Visualization

ℹ️