FSR 0894

(MWSC 714)

0.41 UTI

0.25

C_N

0.2

C_dens

0.5

C_C3

0.55

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 25

Radius (P>50% members) 4.8 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.2 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.55 Moderately studied
C_dup 1.0 Unique

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

Overview

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FSR 0894 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It is moderately studied in the literature.

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

Relatively close High extinction Metal-rich Very young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for FSR 0894 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	–	91.06	20.282	0.281	0.013	-1.136	2.384
Hunt & Reffert	2024	91.134	20.282	0.283	0.005	-1.14	–
Cavallo et al.	2024	91.105	20.303	0.273	–	–	–
Hunt & Reffert	2023	91.134	20.282	0.283	0.005	-1.14	–
Just et al.	2023	91.015	20.281	–	–	–	–
Bica et al.	2019	91.029	20.281	–	–	–	–
Kharchenko et al.	2016	91.015	20.281	–	–	–	–
Kharchenko et al.	2013	91.023	20.28	–	1.0	-7.36	–
Froebrich et al.	2007	91.021	20.281	–	–	–	–
Dias et al.	2002	91.021	20.281	–	1.0	-7.36	–

💡 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	–	–	–	–	–	570*	–	–
Cavallo et al.	2024	3.44	3.54	–	5	0.580	–	–	–
Hunt & Reffert	2023	3.24	4.18	2.73	17	–	–	–	–
Just et al.	2023	–	–	–	16	–	401	–	–
Kharchenko et al.	2016	2.89	3.84	–	16	–	–	–	–
Kharchenko et al.	2013	2.89	3.84	–	16	–	–	–	–
Dias et al.	2002	2.89	3.84	–	16	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 2440	88.0	91.08	20.29	0.29	0.01	-1.15	2.38	0.02

💡 Note: The % column shows the percentage of members that FSR 0894 shares with each listed object.

Visualization

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