FSR 1077

(MWSC 960)

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C3
N_50
r_50
AB 25 1.2
Summary

FSR 1077 is a poorly populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is moderately studied in the literature.

This object shares a large percentage of members with a later reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 100.483 -0.897 0.83 -0.07
Froebrich et al. (2007) 100.483 -0.897
Kharchenko et al. (2012) 100.515 -0.883 0.83 -0.07
Bica et al. (2019) 100.488 -0.898
Hunt & Reffert (2023) 100.471 -0.889 0.195 -0.078 0.572 63.545
Cavallo et al. (2024) 100.486 -0.847 0.194
Hunt & Reffert (2024) 100.471 -0.889 0.195 -0.078 0.572 63.545
           
UCC 100.474 -0.892 0.212 -0.051 0.572
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.416, Dist=1298.0, Age=8.935
Kharchenko et al. (2012) e_bv=0.416, distance=1298, log_age=8.935
Hunt & Reffert (2023) AV50=1.228, diffAV50=1.978, MOD50=13.185, logAge50=8.11
Cavallo et al. (2024) AV50=1.34, dMod50=12.84, logAge50=8.23, [Fe/H]50=-0.01
Hunt & Reffert (2024) MassJ=731.926, MassTot=892.821

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1339 80.0 100.48 -0.86 0.2 -0.02 0.54 0.13