MWSC 2044

0.24 UTI

0.0

C_N

0.02

C_dens

0.12

C_C3

0.52

C_lit

1.0

C_dup

N_m (P>50%) 18

Core radius and density 7.4 [pc], 0.08 [pc^-2]

C3 classification CD

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.12 Very low quality
C_lit 0.52 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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MWSC 2044 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~3.32 kpc) differs significantly from the median photometric distance (~1.17 kpc).

Relatively close Low extinction Intermediate age

Data

🔍 Search references for MWSC 2044 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–	188.267	-60.956	0.301	-2.205	-1.773	–
Just et al.	2023	188.263	-60.927	–	–	–	–
Dib et al.	2018	188.272	-60.93	–	–	–	–
Sampedro et al.	2017	188.25	-60.95	–	-2.34	-1.91	–
Joshi et al.	2016	188.272	-60.93	–	–	–	–
Dias et al.	2016	188.25	-60.95	–	-4.99	-0.48	–
Kharchenko et al.	2016	188.263	-60.927	–	–	–	–
Dias et al.	2014	188.25	-60.95	–	-2.35	-1.95	–
Kharchenko et al.	2013	188.272	-60.93	–	-5.94	-0.75	–
Kharchenko et al.	2009	188.241	-60.951	–	–	–	–
Piskunov et al.	2008	188.241	-60.951	–	–	–	–
Kharchenko et al.	2005	188.25	-60.95	–	-4.99	-0.48	–

💡 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–	1.165	0.5	–	160	–	540	–	–
Just et al.	2023	–	–	–	160	–	126	–	–
Dib et al.	2018	1.23	–	–	160	–	–	–	–
Joshi et al.	2016	1.23	0.50	–	160	–	955	–	–
Dias et al.	2016	1.10	0.50	–	135	–	–	–	–
Kharchenko et al.	2016	1.23	0.50	–	160	–	–	–	–
Kharchenko et al.	2013	1.23	0.50	–	160	–	–	–	–
Kharchenko et al.	2009	1.10	0.50	–	135	–	–	–	–
Piskunov et al.	2008	1.10	0.50	–	135	–	–	–	–
Kharchenko et al.	2005	1.10	0.50	–	135	–	–	–	–

Visualization

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