DBSB 79

(DBS2003 79; MWSC 2067)

0.18 UTI

0.0

C_N

0.0

C_dens

0.38

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 10

Stellar density (N₅₀/rad) 0.0 [N/pc²]

C3 classification BC

C_N 0.0 Sparse
C_dens 0.0 Very loose
C_C3 0.38 Low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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DBSB 79 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very large^* distance, below the mid-plane, affected by high extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~13.26 kpc) differs significantly from the median photometric distance (~1.49 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High extinction Low mass Intermediate age

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.

Data

🔍 Search references for DBSB 79 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–	192.16	-63.771	0.075	-6.754	-0.039	-25.768
Just et al.	2023	192.184	-63.725	–	–	–	–
Kharchenko et al.	2016	192.184	-63.725	–	–	–	–
Kharchenko et al.	2013	192.195	-63.728	–	-11.45	3.81	–
Morales et al.	2013	192.2	-63.743	–	–	–	–

💡 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–	1.49	3.23	–	251	–	12	–	–
Just et al.	2023	–	–	–	251	–	12	–	–
Kharchenko et al.	2016	1.49	3.23	–	251	–	–	–	–
Kharchenko et al.	2013	1.49	3.23	–	251	–	–	–	–

Visualization

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