UPK 160

(OCSN 299)

0.58 UTI

0.29

C_N

1.0

C_dens

1.0

C_C3

0.31

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 29

Radius (P>50% members) 15.4 [arcmin]

C_N 0.29 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

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

Overview

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UPK 160 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Very close Low extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

🔍 Search references for UPK 160 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	–	305.863	64.184	2.097	3.76	0.198	-39.675
Cavallo et al.	2024	307.682	64.113	2.142	–	–	–
Hunt & Reffert	2023	305.699	64.263	2.136	4.061	-0.046	-35.24
Qin et al.	2023	306.77	64.14	2.15	4.13	-0.07	-17.49
He et al.	2022	308.726	64.231	2.166	3.929	-0.164	–
Sim et al.	2019	305.833	64.179	–	3.68	0.29	–

💡 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
Cavallo et al.	2024	0.51	1.45	–	8	0.080	–	–	–
Hunt & Reffert	2023	0.44	0.85	1.80	8	–	–	–	–
Qin et al.	2023	0.70	1.08	–	79	–	–	–	–
He et al.	2022	–	0.60	–	10	–	–	–	–
Sim et al.	2019	0.48	–	–	5	–	–	–	–

Visualization

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