NGC 2678

0.28 UTI

0.0

C_N

0.66

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 21

Radius (P>50% members) 9.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.66 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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NGC 2678 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a close distance, well above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 6 years.

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

Close Low extinction Near-solar metallicity Old

Data

🔍 Search references for NGC 2678 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	–	132.579	11.358	1.049	-10.918	-2.821	35.483
Donor et al.	2020	132.508	11.338	–	-11.01	-3.08	34.1
Dias et al.	2014	132.508	11.338	–	-4.32	-3.55	33.67
Dias et al.	2002	132.508	11.338	–	-4.14	-3.39	33.67

💡 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]	Bfr	BSS
Donor et al.	2020	–	–	–	–	0.000	–	–	–
Dias et al.	2002	0.90	0.09	–	2291	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Melotte 94	92.0	132.85	11.82	1.15	-10.97	-2.91	33.91	1.0
CWWDL 14090	36.0	132.84	11.82	1.15	-10.98	-2.91	33.79	0.0
Chupina 3	4.0	132.85	11.41	1.15	-11.04	-2.83	34.39	0.45

💡 Note: The % column shows the percentage of members that NGC 2678 shares with each listed object.

Visualization

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