Alessi 135

0.00 UTI

0.26

C_N

0.66

C_dens

0.38

C_C3

0.0

C_lit

0.0

C_dup

N_m (P>50%) 26

Core radius and density 1.1 [pc], 3.3 [pc^-2]

C3 classification CB

C_N 0.26 Poorly populated
C_dens 0.66 Moderately dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Alessi 135 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 7 years.

⚠️ 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.

No fundamental parameters

Bica et al. (2019)
List of clusters and alike reported by B. Alessi.

Data

🔍 Search references for Alessi 135 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–	87.412	27.039	1.048	-0.345	-1.033	-3.701
Bica et al.	2019	87.388	27.077	–	–	–	–

💡 Note: The UCC values are estimated from its identified members.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
COIN-Gaia 23	100.0	87.45	27.03	1.05	-0.33	-1.01	-0.01	0.1
Majaess 65	100.0	87.45	27.04	1.04	-0.33	-1.01	-0.05	0.51
CWWDL 14154	96.2	87.46	27.02	1.06	-0.33	-1.0	-3.59	0.01

💡 Note: The % column shows the percentage of members that Alessi 135 shares with each listed object.

Visualization

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