FSR 1335

(MWSC 1448)

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C3
N_50
r_50
AB 40 0.9
Summary

FSR 1335 is a poorly populated, very dense object of high C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is very well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Froebrich et al. (2007) 123.017 -28.981
Kharchenko et al. (2012) 123.001 -29.0 -1.29 4.74
Cantat-Gaudin et al. (2018) 123.012 -28.986 0.131 -2.67 3.172
Bica et al. (2019) 123.026 -28.983
Soubiran et al. (2018) 123.012 -28.986 83.71
Cantat-Gaudin et al. (2020) 123.012 -28.986 0.131 -2.67 3.172
Dias et al. (2021) 123.015 -28.988 0.121 -2.677 3.164
Hunt & Reffert (2023) 123.015 -28.981 0.161 -2.623 3.193 90.91
Cavallo et al. (2024) 123.035 -28.978 0.16
Celli et al. (2024) 123.012 -28.986
Hunt & Reffert (2024) 123.015 -28.981 0.161 -2.623 3.193 90.91
Almeida et al. (2025) 123.015 -28.988
Hu & Soubiran (2025) 123.035 -28.978
           
UCC 123.016 -28.981 0.164 -2.648 3.182 90.912
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
Kharchenko et al. (2012) e_bv=0.562, distance=3835, log_age=9.205
Cantat-Gaudin et al. (2018) dmode=6258.1
Soubiran et al. (2018) dmode=6258.1
Cantat-Gaudin et al. (2020) AVNN=1.03, DistPc=6961.0, AgeNN=7.05
Dias et al. (2021) Av=1.086, Dist=4859, logage=8.234, [Fe/H]=-0.315
Hunt & Reffert (2023) AV50=0.508, diffAV50=1.473, MOD50=13.632, logAge50=8.524
Cavallo et al. (2024) AV50=0.53, dMod50=12.71, logAge50=8.78, [Fe/H]50=-0.52
Celli et al. (2024) Age=11.2, Mc=151.0
Hunt & Reffert (2024) MassJ=329.171, MassTot=350.441
Almeida et al. (2025) AV=1.086, Dist=4859, logAge=8.234, MassRk=145.0
Hu & Soubiran (2025) MA22=-0.33, MA23f=-0.51, MK24=-0.45, MF24=-0.3

Search coordinates in Bayestar19

Cluster region map