DBSB 152

(DBSB2003 152; DBS2003 152)

0.21 UTI

0.58

C_N

0.09

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 66

Core radius and density 2.1 [pc], 0.5 [pc^-2]

C3 classification BC

C_N 0.58 Moderately populated
C_dens 0.09 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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DBSB 152 is a moderately populated, very loose 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 13 years.

⚠️ 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.

No fundamental parameters

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.

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

Data

🔍 Search references for DBSB 152 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–	240.228	-51.606	0.282	-5.249	-3.869	-57.318
Morales et al.	2013	240.229	-51.604	–	–	–	–
Dutra et al.	2003	240.236	-51.605	–	–	–	–

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

Visualization

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