FSR 0999

(MWSC 970)

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0.30 UTI
0.0
CN
0.11
Cdens
0.38
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members) 6.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.38 Low quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

FSR 0999 is a sparse, very loose object of low 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 moderately studied in the literature.

(*): The parallax distance estimate (~3.17 kpc) differs significantly from the median photometric distance (~1.82 kpc).

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 100.929 9.441 0.316 0.592 -1.722
Hunt & Reffert 2024 100.952 9.476 0.303 0.588 -1.723
Cavallo et al. 2024 100.921 9.426 0.302
Hunt & Reffert 2023 100.952 9.476 0.303 0.588 -1.723
Just et al. 2023 100.965 9.427
Bica et al. 2019 100.987 9.436
Kharchenko et al. 2016 100.965 9.427
Kharchenko et al. 2013 100.972 9.425 -0.23 -2.26
Froebrich et al. 2007 100.987 9.432

💡 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 158*
Cavallo et al. 2024 2.33 1.24 309 0.030
Hunt & Reffert 2023 3.15 1.64 0.94 155
Just et al. 2023 708 121
Kharchenko et al. 2016 1.31 1.16 708
Kharchenko et al. 2013 1.31 1.16 708

💡 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.

Visualization

Galactocentric position diagram

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