LP 44

0.17 UTI

0.78

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.34

C_dup

N_m (P>50%) 179

Core radius and density 0.4 [pc], 44 [pc^-2]

C3 classification AB

C_N 0.78 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.34 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

LP 44 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Close Low extinction Very young

Data

🔍 Search references for LP 44 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	100.268	9.555	1.376	-1.989	-3.927	19.602
Loktin & Popova	2017	100.26	9.6	–	-1.239	-7.143	–

💡 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–	0.87	0.23	–	4	–	–	–	–
Loktin & Popova	2017	0.87	0.23	–	4	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
MonOB1-D	66.5	100.25	9.62	1.38	-2.09	-3.7	21.97	0.35
NGC 2264 IRS1	30.2	100.28	9.5	1.37	-2.29	-3.7	20.23	0.5
NGC 2264 IRS1 SE	23.5	100.29	9.49	1.37	-2.31	-3.68	19.6	0.5

💡 Note: The % column shows the percentage of members that LP 44 shares with each listed object.

Visualization

ℹ️