FSR 0288

(MWSC 3468)

0.50 UTI

0.25

C_N

1.0

C_dens

0.5

C_C3

0.38

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 25

Radius (P>50% members) 2.3 [arcmin]

C_N 0.25 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

FSR 0288 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly 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 Moderate 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	–	317.112	49.081	0.319	-2.544	-2.712	-32.539
Hunt & Reffert	2024	317.114	49.09	0.319	-2.529	-2.714	-34.128
Cavallo et al.	2024	317.119	49.097	0.321	–	–	–
Hunt & Reffert	2023	317.114	49.09	0.319	-2.529	-2.714	-34.128
Bica et al.	2019	317.035	49.007	–	–	–	–
Froebrich et al.	2007	317.033	49.002	–	–	–	–
Dias et al.	2002	317.033	49.002	–	-1.85	-4.06	–

💡 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	–	–	–	–	–	355*	–	–
Cavallo et al.	2024	2.84	2.60	–	85	0.210	–	–	–
Hunt & Reffert	2023	2.81	2.48	1.24	192	–	–	–	–
Dias et al.	2002	1.73	2.45	–	295	–	–	–	–

💡 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.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1134	88.0	317.12	49.09	0.33	-2.54	-2.71	-32.54	0.19

💡 Note: The % column shows the percentage of members that FSR 0288 shares with each listed object.

Visualization

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