DBSB 88

(MWSC 2213)

0.16 UTI

0.0

C_N

0.03

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 18

Radius (P>50% members) 5.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.75 High 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 88 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by very high extinction. It is catalogued as a low-mass, young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~6.27 kpc) differs significantly from the median photometric distance (~1.37 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Very high extinction Low mass Young

Data

🔍 Search references for DBSB 88 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	–	215.02	-65.434	0.16	-6.695	-2.965	-65.108
Just et al.	2023	214.892	-65.43	–	–	–	–
Kharchenko et al.	2016	214.892	-65.43	–	–	–	–
Kharchenko et al.	2013	214.905	-65.432	–	-8.43	-3.72	–

💡 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	–	–	–	71	–	29	–	–
Kharchenko et al.	2016	1.37	5.81	–	71	–	–	–	–
Kharchenko et al.	2013	1.37	5.81	–	71	–	–	–	–

Visualization

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