BDSB 62

(BDS2003 62)

0.02 UTI

0.0

C_N

0.1

C_dens

0.38

C_C3

0.0

C_lit

0.16

C_dup

N₅₀ (P>50% members) 16

Stellar density (N₅₀/rad) 0.5 [N/pc²]

C3 classification BC

C_N 0.0 Sparse
C_dens 0.1 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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BDSB 62 is a sparse, very loose object of low 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 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 cluster candidate (IRCC).

Data

🔍 Search references for BDSB 62 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–	60.935	51.003	0.361	-0.343	-0.878	-29.332
Bica et al.	2003	60.957	51.012	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Majaess 42	84.0	60.94	51.0	0.36	-0.32	-0.89	-29.33	0.07

💡 Note: The % column shows the percentage of members that BDSB 62 shares with each listed object.

Visualization

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