FSR 1406

(MWSC 1518)

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0.69 UTI
0.81
CN
1.0
Cdens
0.75
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members) 5.3 [arcmin]
  • CN 0.81 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.44 Poorly studied
  • Cdup 1.0 Unique

Overview

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FSR 1406 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close High extinction Massive Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 129.571 -42.358 0.361 -3.623 2.983 36.904
Hunt & Reffert 2024 129.581 -42.361 0.362 -3.618 2.975 58.434
Cavallo et al. 2024 129.559 -42.359 0.364 – – –
Hunt & Reffert 2023 129.581 -42.361 0.362 -3.618 2.975 58.434
Just et al. 2023 129.565 -42.347 – – – –
Kharchenko et al. 2016 129.565 -42.347 – – – –
Kharchenko et al. 2013 129.57 -42.35 – -3.71 8.1 –
Froebrich et al. 2007 129.588 -42.357 – – – –

💡 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 – – – – – 2008* – –
Cavallo et al. 2024 2.72 4.56 – 174 0.040 – – –
Hunt & Reffert 2023 2.51 4.46 2.90 289 – – – –
Just et al. 2023 – – – 8 – 634 – –
Kharchenko et al. 2016 3.21 4.52 – 8 – – – –
Kharchenko et al. 2013 3.21 4.52 – 8 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1441 39.2 129.57 -42.36 0.36 -3.63 2.98 36.9 0.0

💡 Note: The % column shows the percentage of members that FSR 1406 shares with each listed object.

Visualization

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