ADS 13292

0.37 UTI

0.66

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.76

C_dup

N₅₀ (P>50% members) 83

Stellar density (N₅₀/rad) 260.5 [N/pc²]

C3 classification AB

C_N 0.66 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.76 Very likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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ADS 13292 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 20 years.

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 Moderate extinction Very young

Data

🔍 Search references for ADS 13292 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–	300.598	35.313	0.515	-3.353	-6.713	-5.664
Kronberger et al.	2006	300.597	35.311	–	–	–	–

💡 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–	1.6	1.8	–	10	–	–	–	–
Kronberger et al.	2006	1.60	1.80	–	10	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 8	24.1	300.61	35.31	0.51	-3.39	-6.72	-10.86	0.7

💡 Note: The % column shows the percentage of members that ADS 13292 shares with each listed object.

Visualization

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