CWNU 1310

0.49 UTI

0.51

C_N

0.68

C_dens

0.75

C_C3

0.25

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 52

Radius (P>50% members) 3.3 [arcmin]

C_N 0.51 Moderately populated
C_dens 0.68 Moderately dense
C_C3 0.75 High quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

CWNU 1310 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Distant High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024): Gold sample.

Data

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	300.122	32.796	0.245	-3.14	-5.065	-1.431
Hunt & Reffert	2024	300.086	32.793	0.239	-3.138	-5.055	31.61
Cavallo et al.	2024	300.121	32.8	0.239	–	–	–
Hunt & Reffert	2023	300.086	32.793	0.239	-3.138	-5.055	31.61
He et al.	2023	300.135	32.787	0.243	-3.145	-5.069	-1.43

💡 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
Hunt & Reffert	2024	–	–	–	–	–	376*	–	–
Cavallo et al.	2024	3.27	3.29	–	224	0.360	–	–	–
Hunt & Reffert	2023	3.98	3.23	2.23	102	–	–	–	–
He et al.	2023	3.63	3.45	–	398	–	–	–	–

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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💡 Note: How are the galactocentric plots generated? See FAQ.