DBSB 115

(MWSC 2504)

0.07 UTI

0.38

C_N

1.0

C_dens

0.25

C_C3

0.0

C_lit

0.21

C_dup

N₅₀ (P>50% members) 38

Stellar density (N₅₀/rad) 10.3 [N/pc²]

C3 classification CC

C_N 0.38 Poorly populated
C_dens 1.0 Very dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.21 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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DBSB 115 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close^* distance, above the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~1.65 kpc) differs significantly from the median photometric distance (~2.63 kpc).

Relatively close High extinction Young

Data

🔍 Search references for DBSB 115 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–	254.773	-40.169	0.605	-0.745	-1.01	-15.493
Just et al.	2023	254.802	-40.12	–	–	–	–
Kharchenko et al.	2016	254.802	-40.12	–	–	–	–
Kharchenko et al.	2013	254.812	-40.12	–	-5.6	-3.21	-18.7

💡 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–	2.63	3.87	–	24	–	156	–	–
Just et al.	2023	–	–	–	24	–	156	–	–
Kharchenko et al.	2016	2.63	3.87	–	24	–	–	–	–
Kharchenko et al.	2013	2.63	3.87	–	24	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
DBSB 114	78.9	254.76	-40.2	0.6	-0.32	-1.28	-14.73	0.51
DBSB 117	23.7	254.81	-40.2	0.6	-0.38	-1.32	-15.63	0.28
CWNU 4046	18.4	254.73	-40.2	0.55	-0.15	-1.38	-15.49	0.14

💡 Note: The % column shows the percentage of members that DBSB 115 shares with each listed object.

Visualization

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