DBSB 101

0.00 UTI

0.78

C_N

1.0

C_dens

0.75

C_C3

0.44

C_lit

0.0

C_dup

C3 classification AB

Number of members (P>50%) 183

Radius (P>50% members) 4.6 [arcmin]

C_N 0.78 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.44 Poorly studied
C_dup 0.0 Very likely duplicate

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

Overview

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DBSB 101 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is poorly studied in the literature.

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

Relatively close High extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

🔍 Search references for DBSB 101 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	–	242.61	-49.038	0.536	-1.923	-2.152	-22.899
Hunt & Reffert	2024	242.617	-49.04	0.538	-1.979	-2.173	1.419
Celli et al.	2024	242.631	-49.014	–	–	–	–
Cavallo et al.	2024	242.572	-49.054	0.534	–	–	–
Hunt & Reffert	2023	242.617	-49.04	0.538	-1.979	-2.173	1.419
Cantat-Gaudin et al.	2020	242.631	-49.014	0.52	-1.822	-2.193	–
Cantat-Gaudin & Anders	2020	242.631	-49.014	0.52	-1.822	-2.193	–
Cantat-Gaudin et al.	2018	242.631	-49.014	0.52	-1.822	-2.193	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	1515*	–	–
Celli et al.	2024	–	–	–	11	–	334	–	–
Cavallo et al.	2024	1.55	3.02	–	7	0.050	–	–	–
Hunt & Reffert	2023	1.79	3.26	2.80	4	–	–	–	–
Cantat-Gaudin et al.	2020	1.87	3.07	–	11	–	–	–	–
Cantat-Gaudin & Anders	2020	1.82	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	1.82	–	–	–	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Nor OB5	100.0	242.6	-49.05	0.53	-2.04	-2.15	-23.72	0.62
FSR 1722	98.9	242.6	-49.04	0.53	-2.04	-2.15	-23.72	0.02

💡 Note: The % column shows the percentage of members that DBSB 101 shares with each listed object.

Visualization

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