DB2001 17

(MWSC 3395)

0.45 UTI

0.25

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 25

Radius (P>50% members) 4.3 [arcmin]

C_N 0.25 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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DB2001 17 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 very young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~1.57 kpc) differs significantly from the median photometric distance (~4.23 kpc).

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

Distant Very high extinction Very young

Data

🔍 Search references for DB2001 17 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	–	310.39	41.913	0.636	-2.71	-3.224	-13.701
Just et al.	2023	310.312	41.857	–	–	–	–
Kharchenko et al.	2016	310.312	41.857	–	–	–	–
Kharchenko et al.	2013	310.317	41.86	–	-4.86	-5.82	–

💡 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	–	–	–	3	–	76	–	–
Kharchenko et al.	2016	4.23	6.45	–	3	–	–	–	–
Kharchenko et al.	2013	4.23	6.45	–	3	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
DB2001 18	72.0	310.36	41.96	0.66	-2.7	-3.1	-13.7	0.4

💡 Note: The % column shows the percentage of members that DB2001 17 shares with each listed object.

Visualization

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