Czernik 45

(MWSC 3776; OCL 278)

0.63 UTI

0.66

C_N

1.0

C_dens

0.75

C_C3

0.38

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 81

Radius (P>50% members) 1.2 [arcmin]

C_N 0.66 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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Czernik 45 is a moderately populated, very 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 young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.07 kpc) differs significantly from the median photometric distance (~2.50 kpc).

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

Relatively close High extinction Young

Data

🔍 Search references for Czernik 45 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	–	358.928	64.62	0.245	-2.411	-0.781	44.154
Just et al.	2023	358.948	64.616	–	–	–	–
Bica et al.	2019	358.943	64.62	–	–	–	–
Kharchenko et al.	2016	358.948	64.616	–	–	–	–
Dias et al.	2014	359.075	64.55	–	-3.09	1.04	–
Kharchenko et al.	2013	358.957	64.62	–	-6.03	-7.14	-79.8
Kharchenko et al.	2012	358.957	64.62	–	-6.03	-7.14	-79.8

💡 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
Just et al.	2023	–	–	–	51	–	68	–	–
Kharchenko et al.	2016	2.50	3.56	–	51	–	–	–	–
Kharchenko et al.	2013	2.50	3.56	–	51	–	–	–	–
Kharchenko et al.	2012	2.50	3.56	–	51	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1192	64.2	358.93	64.62	0.24	-2.43	-0.78	44.15	0.0

💡 Note: The % column shows the percentage of members that Czernik 45 shares with each listed object.

Visualization

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