FSR 1744

(SAI 124; MWSC 2474)

0.74 UTI

0.58

C_N

1.0

C_dens

1.0

C_C3

0.56

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 67

Radius (P>50% members) 4.6 [arcmin]

C_N 0.58 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.56 Moderately studied
C_dup 1.0 Unique

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

Overview

FSR 1744 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

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

Relatively close High extinction Metal-poor Intermediate age

Cavallo et al. (2024): Bronze sample.

Data

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	252.958	-42.407	0.59	0.254	-0.137	-2.885
Hunt & Reffert	2024	252.973	-42.409	0.576	0.266	-0.131	-24.16
Cavallo et al.	2024	252.939	-42.414	0.576	–	–	–
Hunt & Reffert	2023	252.973	-42.409	0.576	0.266	-0.131	-24.16
Just et al.	2023	252.874	-42.393	–	–	–	–
Bica et al.	2019	252.902	-42.411	–	–	–	–
Kharchenko et al.	2016	252.874	-42.393	–	–	–	–
Kharchenko et al.	2013	252.885	-42.393	–	-3.05	-3.15	–
Glushkova et al.	2010	252.899	-42.43	–	–	–	–
Froebrich et al.	2007	252.9	-42.415	–	–	–	–

💡 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	–	–	–	–	–	450*	–	–
Cavallo et al.	2024	2.49	2.08	–	324	-0.730	–	–	–
Hunt & Reffert	2023	1.60	1.83	2.29	163	–	–	–	–
Just et al.	2023	–	–	–	398	–	54	–	–
Kharchenko et al.	2016	1.84	3.10	–	398	–	–	–	–
Kharchenko et al.	2013	1.84	3.10	–	398	–	–	–	–
Glushkova et al.	2010	3.13	8.00	–	708	–	–	–	–

💡 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 1560	65.7	252.96	-42.41	0.6	0.25	-0.14	-2.88	0.0

💡 Note: The % column shows the percentage of members that FSR 1744 shares with each listed object.

Visualization

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