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

Bica et al. (2019)
Asterisms reported by amateur astronomers in the web. The Preliminary Amateur Open Cluster Catalog, Version 08/03/2003.

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	1.83	–	10	–	–	–	–
Kronberger et al.	2006	1.60	1.83	–	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	0.61

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

Visualization

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