GGD17

0.43 UTI

0.51

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 52

Stellar density (N₅₀/rad) 47.8 [N/pc²]

C3 classification AC

C_N 0.51 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate 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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GGD17 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a close distance, below 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 23 years.

Note: This object shares a small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

No fundamental parameters

Bica et al. (2003)
Classified as infrared cluster (IRC).

Data

🔍 Search references for GGD17 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–	93.192	-6.251	1.143	-3.854	0.449	37.031
Bica et al.	2003	93.196	-6.23	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 2183	23.1	92.69	-6.24	1.19	-3.63	0.4	25.06	0.82
OC 0358	11.5	93.11	-6.38	1.17	-3.88	0.35	27.82	0.19

💡 Note: The % column shows the percentage of members that GGD17 shares with each listed object.

Visualization

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