BDSB 67

(BDS2003 67)

0.07 UTI

0.47

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.19

C_dup

N₅₀ (P>50% members) 47

Stellar density (N₅₀/rad) 5.2 [N/pc²]

C3 classification BC

C_N 0.47 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.19 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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BDSB 67 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above 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

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

Data

🔍 Search references for BDSB 67 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–	70.164	50.461	0.204	-0.091	-0.442	19.157
Bica et al.	2003	70.156	50.461	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 1624	80.9	70.16	50.46	0.19	-0.05	-0.44	19.16	0.64

💡 Note: The % column shows the percentage of members that BDSB 67 shares with each listed object.

Visualization

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