MDF2011 cl1

0.02 UTI

0.0

C_N

0.08

C_dens

0.12

C_C3

0.0

C_lit

0.4

C_dup

N₅₀ (P>50% members) 18

Stellar density (N₅₀/rad) 0.4 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.08 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.4 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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MDF2011 cl1 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 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.

(*): The parallax distance estimate (~2.64 kpc) differs significantly from the median photometric distance (~3.79 kpc).

Distant

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, presence of an IR bubble.

Data

🔍 Search references for MDF2011 cl1 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–	273.544	-17.973	0.378	-0.83	-1.498	24.906
Morales et al.	2013	273.592	-17.936	–	–	–	–

💡 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–	3.79	–	–	–	–	–	–	–
Morales et al.	2013	3.79	–	–	–	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
MCM 1	60.0	273.48	-17.94	0.43	-0.84	-1.52	47.03	0.11

💡 Note: The % column shows the percentage of members that MDF2011 cl1 shares with each listed object.

Visualization

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