DBSB 128

(DBSB2003 128)

0.13 UTI

0.6

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.27

C_dup

N₅₀ (P>50% members) 71

Stellar density (N₅₀/rad) 6.6 [N/pc²]

C3 classification AB

C_N 0.6 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.27 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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DBSB 128 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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 infrared cluster (IRC).

Data

🔍 Search references for DBSB 128 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–	159.364	-58.668	0.381	-7.024	2.758	-49.584
Dutra et al.	2003	159.504	-58.774	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 3324	73.2	159.33	-58.62	0.37	-7.08	2.8	-21.01	0.91

💡 Note: The % column shows the percentage of members that DBSB 128 shares with each listed object.

Visualization

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