DBSB 79

(DBSB2003 79; DBS2003 79; MWSC 2067)

0.14 UTI

0.0

C_N

0.0

C_dens

0.38

C_C3

0.16

C_lit

1.0

C_dup

N_m (P>50%) 10

Core radius and density 13 [pc], 0.01 [pc^-2]

C3 classification BC

C_N 0.0 Sparse
C_dens 0.0 Very loose
C_C3 0.38 Low quality
C_lit 0.16 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

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 rarely 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.

Dutra et al. (2003)
Classified as infrared cluster (IRC).

Data

🔍 Search references for DBSB 79 in: SciX Simbad

ℹ️

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	–	–	–	–
Dib et al.	2018	192.195	-63.728	–	–	–	–
Joshi et al.	2016	192.195	-63.728	–	–	–	–
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	–	–	–	–
Dutra et al.	2003	192.2	-63.74	–	–	–	–

💡 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	3.28	–	251	–	12	–	–
Just et al.	2023	–	–	–	251	–	12	–	–
Dib et al.	2018	1.49	–	–	251	–	–	–	–
Joshi et al.	2016	1.49	3.28	–	251	–	–	–	–
Kharchenko et al.	2016	1.49	3.28	–	251	–	–	–	–
Kharchenko et al.	2013	1.49	3.28	–	251	–	–	–	–

Visualization

ℹ️