DBSB 11

(DBSB2003 11)

0.16 UTI

0.75

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.33

C_dup

N₅₀ (P>50% members) 104

Stellar density (N₅₀/rad) 107.3 [N/pc²]

C3 classification AC

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.33 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

DBSB 11 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close 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 possibly a duplicate object, which shares a significant 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 11 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	111.067	-24.639	0.709	-2.086	2.557	18.636
Dutra et al.	2003	111.062	-24.632	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Ivanov 6	67.3	111.06	-24.64	0.72	-2.05	2.69	18.64	0.66
CWNU 1337	6.7	111.03	-24.4	0.72	-2.14	2.23	31.62	0.18
Majaess 90	6.7	111.19	-24.48	0.74	-2.16	2.27	31.62	0.42

💡 Note: The % column shows the percentage of members that DBSB 11 shares with each listed object.

Visualization

ℹ️