FSR 0413

(MWSC 3687)

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0.38 UTI
0.0
CN
1.0
Cdens
0.12
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 6.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.12 Very low quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

FSR 0413 is a sparse, very dense object of very low C3 quality. Its parallax locates it at a close* distance, above the mid-plane, affected by high extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~0.96 kpc) differs significantly from the median photometric distance (~1.80 kpc).

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

Relatively close High extinction Low mass Intermediate age

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 345.141 62.891 1.046 -2.239 -2.563 2.423
Just et al. 2023 345.202 62.884
Kharchenko et al. 2016 345.202 62.884
Kharchenko et al. 2013 345.21 62.888 -4.95 -2.17
Kharchenko et al. 2012 345.21 62.888 -4.95 -2.17
Froebrich et al. 2007 345.25 62.894
Dias et al. 2002 345.25 62.894 -4.95 -2.17

💡 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
Just et al. 2023 178 6
Kharchenko et al. 2016 1.80 4.80 178
Kharchenko et al. 2013 1.80 4.80 178
Kharchenko et al. 2012 1.80 4.80 178
Dias et al. 2002 1.80 4.80 178

💡 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.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 4 24.0 344.35 62.99 1.16 -2.4 -2.56 -13.56 0.47

💡 Note: The % column shows the percentage of members that FSR 0413 shares with each listed object.

Visualization

Galactocentric position diagram

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