VVV 035

(VVV-CL 035)

0.10 UTI

0.3

C_N

0.05

C_dens

0.12

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 30

Core radius and density 1.9 [pc], 0.3 [pc^-2]

C3 classification DC

C_N 0.3 Poorly populated
C_dens 0.05 Very loose
C_C3 0.12 Very 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

ℹ️

VVV 035 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate 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 13 years.

Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.

⚠️ 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

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, presence of emission related to PAH or warm dust.

Data

🔍 Search references for VVV 035 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	211.61	-61.455	0.35	-7.689	-2.826	-51.933
Morales et al.	2013	211.613	-61.493	–	–	–	–
Borissova et al.	2011	211.613	-61.493	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
LS 139	3.3	211.52	-61.57	0.39	-7.46	-2.6	-22.87	0.1

💡 Note: The % column shows the percentage of members that VVV 035 shares with each listed object.

Visualization

ℹ️