DBSB 62

(MWSC 1910)

0.27 UTI

0.75

C_N

0.23

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 103

Radius (P>50% members) 4.8 [arcmin]

C_N 0.75 Rich
C_dens 0.23 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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DBSB 62 is a rich, very loose object of low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by low extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~6.82 kpc) differs significantly from the median photometric distance (~2.19 kpc).

Relatively close Low extinction Very young

Data

🔍 Search references for DBSB 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	–	167.754	-61.222	0.147	-6.375	1.907	-0.934
Just et al.	2023	167.827	-61.286	–	–	–	–
Kharchenko et al.	2016	167.827	-61.286	–	–	–	–
Kharchenko et al.	2013	167.835	-61.29	–	-4.62	4.33	-15.6

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

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Just et al.	2023	–	–	–	8	–	242	–	–
Kharchenko et al.	2016	2.19	0.97	–	8	–	–	–	–
Kharchenko et al.	2013	2.19	0.97	–	8	–	–	–	–

Visualization

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