DBSB 36

(MWSC 1645)

0.62 UTI

0.36

C_N

1.0

C_dens

1.0

C_C3

0.38

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 36

Radius (P>50% members) 1.8 [arcmin]

C_N 0.36 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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DBSB 36 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close^* distance, near the mid-plane, affected by very high extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~1.76 kpc) differs significantly from the median photometric distance (~1.18 kpc).

Relatively close Very high extinction Metal-rich Young

Cavallo et al. (2024)
Wood sample.

Data

🔍 Search references for DBSB 36 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	–	139.193	-47.953	0.569	-5.138	4.219	93.608
Hunt & Reffert	2024	139.188	-47.95	0.583	-5.128	4.203	93.615
Cavallo et al.	2024	139.163	-47.942	0.587	–	–	–
Hunt & Reffert	2023	139.188	-47.95	0.583	-5.128	4.203	93.615
Just et al.	2023	139.195	-47.942	–	–	–	–
Kharchenko et al.	2016	139.195	-47.942	–	–	–	–
Kharchenko et al.	2013	139.2	-47.945	–	-5.36	6.99	21.0

💡 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	–	–	–	–	–	311*	–	–
Cavallo et al.	2024	2.98	4.95	–	102	0.570	–	–	–
Hunt & Reffert	2023	1.60	5.24	2.75	98	–	–	–	–
Just et al.	2023	–	–	–	32	–	11	–	–
Kharchenko et al.	2016	0.75	7.03	–	32	–	–	–	–
Kharchenko et al.	2013	0.75	7.03	–	32	–	–	–	–

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

Visualization

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