DBSB 175

(MWSC 2478)

0.05 UTI

0.0

C_N

0.12

C_dens

0.12

C_C3

0.0

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 16

Radius (P>50% members) 7.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.12 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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DBSB 175 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~2.42 kpc) differs significantly from the median photometric distance (~3.80 kpc).

Note: This object shares a small percentage of members with 2 later reported entries. See table with shared members information.

⚠️ 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.

Distant High extinction Very young

Data

🔍 Search references for DBSB 175 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	–	253.065	-43.421	0.414	-1.262	-3.815	-23.938
Just et al.	2023	253.137	-43.396	–	–	–	–
Kharchenko et al.	2016	253.137	-43.396	–	–	–	–
Kharchenko et al.	2013	253.147	-43.396	–	-2.69	-2.03	-45.9

💡 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]	Bfr	BSS
Just et al.	2023	–	–	–	1	–	632	–	–
Kharchenko et al.	2016	3.80	3.87	–	1	–	–	–	–
Kharchenko et al.	2013	3.80	3.87	–	1	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Bica 513	20.0	253.42	-43.52	0.44	-1.4	-3.84	-16.7	0.08
Ryu 82	4.0	253.17	-43.2	0.44	-1.39	-3.38	-17.67	0.22

💡 Note: The % column shows the percentage of members that DBSB 175 shares with each listed object.

Visualization

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