DBSB 144

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C3
N_50
r_50
BA 30 4.5
Summary

DBSB 144 is a poorly populated, moderately dense object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is poorly 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
Kharchenko et al. (2012) 243.041 -51.475 -5.98 -0.94
Hunt & Reffert (2023) 243.021 -51.465 0.446 -1.695 -1.947 -42.594
Cavallo et al. (2024) 243.048 -51.502 0.447
Hunt & Reffert (2024) 243.021 -51.465 0.446 -1.695 -1.947 -42.594
           
UCC 243.047 -51.487 0.436 -1.683 -1.923 -43.241
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=0.979, distance=7362, log_age=6.0
Hunt & Reffert (2023) AV50=1.768, diffAV50=0.685, MOD50=11.615, logAge50=7.97
Cavallo et al. (2024) AV50=1.69, dMod50=11.14, logAge50=8.34, [Fe/H]50=-0.13
Hunt & Reffert (2024) MassJ=309.716, MassTot=309.716

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 539 86.7 243.06 -51.48 0.43 -1.67 -1.92 -43.24 0.11