IRAS 20264+4042

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.4 0.3 0.75 0.0 0.98
C3
N_50
r_50
AB 40 9.1
Summary

IRAS 20264+4042 is a poorly populated, loose object of high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Kharchenko et al. (2012) 307.058 40.885 – -1.32 -1.14 –
           
UCC 307.061 40.824 0.512 -2.023 -4.355 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

IRAS 20264+4042 UCC

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Fundamental parameters

Reference Values
Kharchenko et al. (2012) e_bv=0.937, distance=1818, log_age=6.6

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Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Bica 136 25.0 307.26 40.49 0.51 -1.84 -4.54 – 0.39
FSR 0227 2.5 307.26 40.48 0.63 -1.92 -4.38 – 0.46