Mandushev 1

0.05 UTI

0.0

C_N

0.01

C_dens

0.25

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 13

Core radius and density 9.6 [pc], 0.04 [pc^-2]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Mandushev 1 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, above 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 24 years.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

No fundamental parameters

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). Web updates in DAML02, some were later removed (2003 to 2010).

Dias et al. (2016)
Asterism (Turner, D. G. et al. 1998, JRASC 92, 145); cat V3.5 (Jan 2016)

Data

🔍 Search references for Mandushev 1 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–	295.494	29.443	0.191	-2.306	-5.618	-9.535
Dias et al.	2002	295.5	29.452	–	–	–	–

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

Visualization

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