DBSB 88

(DBSB2003 88; MCM 50; MCM2005b 50; DBS2003 88; MWSC 2213)

0.27 UTI

0.76

C_N

1.0

C_dens

0.75

C_C3

0.29

C_lit

0.43

C_dup

N₅₀ (P>50% members) 122

Stellar density (N₅₀/rad) 32.9 [N/pc²]

C3 classification AB

C_N 0.76 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.29 Poorly studied
C_dup 0.43 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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DBSB 88 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by very high extinction. It is catalogued as a low-mass, young cluster (see Parameters). It is poorly studied in the literature.

⚠️ 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.

Relatively close Very high extinction Low mass Young

Mercer et al. (2005)
Associated with mid-IR extended emission. Cluster of stars. Detected using no magnitude cut. Detected in 2MASS catalog with our algorithm.

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, presence of an IR bubble.

Dutra et al. (2003)
Classified as stellar group (IRGr).

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	99999–	214.82	-61.431	0.574	-3.252	-3.095	-41.325
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	–
Morales et al.	2013	214.915	-61.422	–	–	–	–
Mercer et al.	2005	214.913	-61.422	–	–	–	–
Dutra et al.	2003	214.917	-65.427	–	–	–	–

💡 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]	B_frac	BSS
UCC	99999–	1.37	5.81	–	71	–	29	–	–
Just et al.	2023	–	–	–	71	–	29	–	–
Kharchenko et al.	2016	1.37	5.81	–	71	–	–	–	–
Kharchenko et al.	2013	1.37	5.81	–	71	–	–	–	–
Morales et al.	2013	1.82	–	–	1	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Loden 1256	56.6	214.77	-61.43	0.58	-3.28	-3.11	-55.63	0.65
OC 0608	20.5	214.85	-61.43	0.59	-3.19	-3.14	-55.63	0.0

💡 Note: The % column shows the percentage of members that DBSB 88 shares with each listed object.

Visualization

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