FSR 0377

(MWSC 3641)

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0.43 UTI
0.59
CN
0.23
Cdens
0.75
CC3
0.29
Clit
1.0
Cdup
Core radius and density 2.0 [pc], 1.2 [pc-2]
  • CN 0.59 Moderately populated
  • Cdens 0.23 Very loose
  • CC3 0.75 High quality
  • Clit 0.29 Poorly studied
  • Cdup 1.0 Unique

Overview

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FSR 0377 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.54 kpc) differs significantly from the median photometric distance (~2.30 kpc).

Note: This object shares a moderate percentage of members with 2 later reported entries. See table with shared members information.

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 338.726 58.296 0.22 -3.287 -2.168 -63.881
Almeida et al. 2025 338.719 58.304 – – – –
Just et al. 2023 338.649 58.292 – – – –
Dias et al. 2021 338.719 58.304 0.207 -3.219 -2.155 –
Bica et al. 2019 338.71 58.308 – – – –
Sampedro et al. 2017 338.717 58.304 – -2.55 -5.6 –
Kharchenko et al. 2016 338.649 58.292 – – – –
Dias et al. 2014 338.717 58.304 – -5.88 -4.04 –
Kharchenko et al. 2013 338.655 58.295 – -4.58 -1.53 –
Kharchenko et al. 2012 338.655 58.295 – -4.58 -1.53 –
Froebrich et al. 2007 338.717 58.304 – – – –
Dias et al. 2002 338.717 58.304 – -5.87 -4.04 –

💡 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] Bfrac BSS
UCC 99999– 2.3 1.89 – 50 -0.065 304 – –
Almeida et al. 2025 3.56 2.16 – 12 – 583 – –
Just et al. 2023 – – – 50 – 26 – –
Dias et al. 2021 3.56 2.16 – 12 -0.065 – – –
Kharchenko et al. 2016 2.30 1.89 – 50 – – – –
Kharchenko et al. 2013 2.30 1.89 – 50 – – – –
Kharchenko et al. 2012 2.30 1.89 – 50 – – – –
Dias et al. 2002 2.30 1.89 – 50 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 390 44.1 338.71 58.29 0.22 -3.38 -2.15 -8.54 0.06
Sh2-138 2.9 338.17 58.51 0.26 -3.27 -2.14 -70.89 0.05

💡 Note: The % column shows the percentage of members that FSR 0377 shares with each listed object.

Visualization

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