FSR 0480

(SAI 3; MWSC 25)

0.83 UTI

0.82

C_N

1.0

C_dens

0.75

C_C3

0.79

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 282

Radius (P>50% members) 3.4 [arcmin]

C_N 0.82 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.79 Well-studied
C_dup 1.0 Unique

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Overview

FSR 0480 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster (see Parameters). It is well-studied in the literature.

Very distant Moderate extinction Massive Near-solar metallicity Old

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	–	3.726	61.491	0.178	-2.772	-0.345	-52.534
Hu & Soubiran	2025	3.72	61.507	–	–	–	–
Hunt & Reffert	2024	3.775	61.509	0.165	-2.772	-0.342	-52.136
Cavallo et al.	2024	3.72	61.507	0.169	–	–	–
He et al.	2023	3.722	61.492	0.169	-2.779	-0.344	-52.56
Hunt & Reffert	2023	3.775	61.509	0.165	-2.772	-0.342	-52.136
Just et al.	2023	3.727	61.468	–	–	–	–
Bica et al.	2019	3.719	61.472	–	–	–	–
Kharchenko et al.	2016	3.727	61.468	–	–	–	–
Kharchenko et al.	2013	3.736	61.471	–	-0.31	-2.33	–
Kharchenko et al.	2012	3.736	61.471	–	-0.14	-1.97	–
Glushkova et al.	2010	3.707	61.477	–	–	–	–
Froebrich et al.	2007	3.729	61.473	–	–	–	–
Dias et al.	2002	3.729	61.473	–	-1.66	-1.81	–

💡 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
Hu & Soubiran	2025	–	–	–	–	-0.410*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	3063*	–	–
Cavallo et al.	2024	6.37	2.84	–	2089	-0.500	–	–	–
He et al.	2023	5.01	3.10	–	1585	–	–	–	–
Hunt & Reffert	2023	4.90	3.21	2.19	668	–	–	–	–
Just et al.	2023	–	–	–	1995	–	1849	–	–
Kharchenko et al.	2016	5.49	2.90	–	1995	–	–	–	–
Kharchenko et al.	2013	5.49	2.90	–	1995	–	–	–	–
Kharchenko et al.	2012	5.49	2.90	–	1995	–	–	–	–
Glushkova et al.	2010	6.90	2.11	–	1585	–	–	–	–
Dias et al.	2002	5.49	2.90	–	1995	–	–	–	–

💡 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.

Visualization

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