DBSB 117

(DBSB2003 117; DBS2003 117)

0.28 UTI

0.0

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 22

Core radius and density 0.7 [pc], 9.7 [pc^-2]

C3 classification BC

C_N 0.0 Sparse
C_dens 1.0 Very dense
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 117 is a sparse, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

Note: This object shares a large percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, presence of emission related to PAH or warm dust.

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

Data

🔍 Search references for DBSB 117 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–	254.809	-40.201	0.6	-0.375	-1.325	-15.633
Morales et al.	2013	254.912	-40.189	–	–	–	–
Dutra et al.	2003	254.91	-40.186	–	–	–	–

💡 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–	1.61	–	–	–	–	–	–	–
Morales et al.	2013	1.61	–	–	–	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
DBSB 114	92.0	254.76	-40.2	0.6	-0.32	-1.28	-14.73	0.51
CWNU 4046	56.0	254.73	-40.2	0.55	-0.15	-1.38	-15.49	0.12
DBSB 115	36.0	254.77	-40.17	0.6	-0.75	-1.01	-15.49	0.24

💡 Note: The % column shows the percentage of members that DBSB 117 shares with each listed object.

Visualization

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