FSR 1430

(SAI 96; MWSC 1589)

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0.75 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.62
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.62 Moderately studied
  • Cdup 1.0 Unique

Overview

FSR 1430 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Very distant Very high extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024): Bronze sample.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 132.966 -44.271 0.18 -3.676 2.722 96.622
Hunt & Reffert 2024 132.976 -44.277 0.179 -3.691 2.733 96.665
Cavallo et al. 2024 132.957 -44.278 0.192
He et al. 2023 132.971 -44.273 0.181 -3.7 2.731 96.62
Hunt & Reffert 2023 132.976 -44.277 0.179 -3.691 2.733 96.665
Just et al. 2023 132.962 -44.25
Kharchenko et al. 2016 132.962 -44.25
Kharchenko et al. 2013 132.967 -44.253 -11.48 6.06
Glushkova et al. 2010 132.956 -44.263
Froebrich et al. 2007 132.967 -44.266
Dias et al. 2002 132.954 -44.263 0.26 2.8

💡 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 3304*
Cavallo et al. 2024 9.46 4.87 1380 -0.240
He et al. 2023 5.75 6.50 631
Hunt & Reffert 2023 4.56 6.04 2.25 1007
Just et al. 2023 316 4140
Kharchenko et al. 2016 6.74 8.26 316
Kharchenko et al. 2013 6.74 8.26 316
Glushkova et al. 2010 2.84 7.75 708
Dias et al. 2002 2.84 7.75 708

💡 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.