DBSB 15

(DBSB2003 15)

0.05 UTI

0.34

C_N

0.22

C_dens

0.5

C_C3

0.0

C_lit

0.24

C_dup

N₅₀ (P>50% members) 34

Stellar density (N₅₀/rad) 1.1 [N/pc²]

C3 classification BB

C_N 0.34 Poorly populated
C_dens 0.22 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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DBSB 15 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 23 years.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

No fundamental parameters

Dutra et al. (2003)
Classified as open cluster (IROC).

Data

🔍 Search references for DBSB 15 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–	115.071	-33.56	0.259	-2.254	3.054	–
Dutra et al.	2003	115.079	-33.545	–	–	–	–

💡 Note: The UCC values are estimated from its identified members.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3351	91.2	115.07	-33.57	0.26	-2.25	3.04	–	0.05
Bochum 15	76.5	115.08	-33.57	0.26	-2.24	3.04	–	0.31
Cmg 1050	20.6	114.86	-33.65	0.26	-2.24	3.03	–	0.06

💡 Note: The % column shows the percentage of members that DBSB 15 shares with each listed object.

Visualization

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