Harris / Gaia EDR3 Globulars · 4 Profiled Objects

Milky Way Globular Clusters Reference Catalog

Astrometric and photometric reference index for Galactic globular clusters, linking Shapley-Sawyer classes, metallicities [Fe/H], and Gaia distances.

Compiler & Survey Epoch: W. E. Harris (1996/2010) & Vasiliev / Baumgardt (2021 Gaia EDR3)

Catalog Scope & Cross-Identification Notes

The Catalog of Parameters for Milky Way Globular Clusters compiled by William E. Harris and updated with Gaia EDR3 proper motions and parallaxes by Vasiliev & Baumgardt (2021) serves as the standard benchmark for studying the ancient stellar halo of our galaxy.

This cross-walk links FastAstro's flagship northern and southern globular cluster profiles with their NGC/Messier designations, Shapley-Sawyer core concentrations, metallicities, and horizontal-branch distances.

Cross-Referenced Objects in Milky Way Globular Clusters Reference Catalog (4)

Cross-referenced celestial objects in Milky Way Globular Clusters Reference Catalog
Object ProfilePrimary ClassConstellationRA (J2000)Dec (J2000)Catalog AliasesBest Season
Messier 13 (Hercules Globular Cluster)Globular clusterHercules16h 41m 41.24s+36° 27′ 35.5″M13, NGC 6205, Hercules Globular ClusterLate Spring to Summer (May–August)
Omega Centauri (NGC 5139 Cluster)Globular cluster / stripped dwarf galaxy nucleusCentaurus13h 26m 47.24s-47° 28′ 46.1″ω Centauri, NGC 5139, Caldwell 80Spring to Early Summer (April–June)
Messier 92 (NGC 6341 in Hercules)Globular clusterHercules17h 17m 07.40s+43° 08′ 09.4″M92, NGC 6341Late Spring to Summer (May–August)
47 Tucanae (NGC 104 Globular Cluster)Globular clusterTucana (Southern Sky)00h 24m 05.30s-72° 04′ 52.6″47 Tuc, NGC 104, Caldwell 106Southern Spring to Summer (September–December)
Reference Guide

Trigonometric Parallax, Parsecs & Gaia DR3

How trigonometric parallax (d_pc = 1 / p_arcsec), the distance modulus equation, Hipparcos, and Gaia DR3 microarcsecond astrometry measure cosmic distances.

Reference Guide

Apparent vs Absolute Magnitude Explained

Understand the logarithmic Pogson astronomical magnitude scale, apparent visual magnitude (m), absolute magnitude (M at 10 parsecs), and bolometric corrections.

Primary Catalog Sources