DBSB 35

(MWSC 1641)

0.31 UTI

0.57

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.75

C_dup

C3 classification BB

Number of members (P>50%) 64

Radius (P>50% members) 2.4 [arcmin]

C_N 0.57 Moderately populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.75 Very likely unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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DBSB 35 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close High extinction Very young

Data

🔍 Search references for DBSB 35 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	–	138.786	-47.469	0.593	-5.317	4.228	63.621
Just et al.	2023	138.785	-47.461	–	–	–	–
Kharchenko et al.	2016	138.785	-47.461	–	–	–	–
Kharchenko et al.	2013	138.79	-47.465	–	-6.98	9.98	–

💡 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	–	–	–	6	–	61	–	–
Kharchenko et al.	2016	1.68	4.58	–	6	–	–	–	–
Kharchenko et al.	2013	1.68	4.58	–	6	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 102	25.0	138.8	-47.49	0.6	-5.26	4.28	63.62	0.25

💡 Note: The % column shows the percentage of members that DBSB 35 shares with each listed object.

Visualization

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