Galactic Globular Cluster Research Portal银河系球状星团研究门户

Milky Way Globular Cluster Atlas银河系球状星团图谱

One catalog, 176 ancient star cities, three equal ways in. The unified atlas cross-matches five surveys, integrates 135 orbits against MWPotential2014, tracks 124 stellar streams, and models the spiral arms & bar — served through a 3D explorer, a plotting bench, and a knowledge base. 一份星表,176 座古老星城,三种平等的进入方式。本图谱交叉匹配五份巡天数据,在 MWPotential2014 势场下积分 135 条轨道,追踪 124 条恒星流,并建模旋臂与中央棒——通过 3D 浏览器、制图台与知识库呈现。

Galactic coordinates · Aitoff projection银道坐标 · Aitoff 投影 J2000
[Fe/H]−2.5−1+0.5
click-free hover · real positions from master_catalog悬停查看 · 真实位置取自统一星表
176 globular clusters球状星团· 135 integrated orbits已积分轨道· 124 stellar streams恒星流· 4+2 spiral arms + bar旋臂 + 棒· 5 surveys数据巡天
Three Equal Instruments三个平权模块

One observatory, three rooms一座天文台,三个房间

The dome is for roaming the sky, the bench for drawing figures, the library for reading the literature — three rooms, each with its own duty, none above another. 圆顶用来漫游天空,测量台用来绘制图件,书房用来研读文献——三个房间各司其职,不分主次。

Strung together, they trace the full course of studying a cluster system: first see it, then measure it, at last understand it. 串起来看,它们恰好是研究一群星团的完整过程:先看见,再量清,后读懂。

Common ground — all three rooms read the same unified catalog:共同地基 —— 三个房间读取同一份统一星表: master_catalog · 39 fields · 176 objects View the data →查看数据 →

Data Foundation数据基础

176 Milky Way globular clusters, cross-identified and merged from four authoritative catalogs. Names are normalized (Messier/common aliases → Harris primary key) and matched by coordinates (3″ tolerance); multi-source fields are fused by precision priority. 135 clusters have full 6-D phase space (position + proper motion + radial velocity). 176 个银河系球状星团,经交叉比对并从四份权威星表合并而成。名称已规范化(梅西耶/常用别名 → Harris 主键),并按坐标(3″ 容差)匹配;多源字段按精度优先级融合。其中 135 个星团具备完整的 6 维相空间(位置 + 自行 + 视向速度)。

Field coverage字段覆盖Count数量
Distance距离170
Proper motion (Gaia EDR3)自行(Gaia EDR3)170
Mass质量118
Metallicity [Fe/H]金属丰度 [Fe/H]139
Radial velocity视向速度141
Full 6-D phase space完整 6 维相空间135
Merge priority — distance: Baumgardt&Hilker > Gaia parallax > Harris; coordinates/PM from Gaia EDR3; metallicity from Harris; mass/structure from Baumgardt & Hilker.合并优先级——距离:Baumgardt&Hilker > Gaia 视差 > Harris;坐标/自行取自 Gaia EDR3;金属丰度取自 Harris;质量/结构取自 Baumgardt & Hilker。
Spot-check clusters抽样核对星团Distance距离[Fe/H]ecc偏心率
47 Tuc (NGC 104)4.41 kpc−0.760.12
ω Cen (NGC 5139)5.20 kpc−1.620.69
M13 (NGC 6205)6.60 kpc−1.540.81
Values match the literature exactly. ω Cen (3.55×10⁶ M☉) is the most massive Galactic globular cluster.数值与文献完全一致。ω Cen(3.55×10⁶ M☉)是银河系中质量最大的球状星团。
master_catalog.csv master_catalog.json orbits.json 39 fields

Sources & References来源与参考文献 VizieR verified

Every catalog was verified against its official CDS VizieR identifier and is cited with its original reference. Click any card to open the source. Data remain the property of their respective authors/institutions and are redistributed here for research and educational use. 每份星表均经官方 CDS VizieR 编号核验,并附原始文献引用。点击任意卡片可打开来源。数据归各自作者/机构所有,此处仅用于研究与教育用途再分发。

Harris 1996 / 2010
VizieR VII/202/catalog
The standard GC catalog: coordinates, distances, photometry, [Fe/H], E(B−V), radial velocities, structure, relaxation times, central densities (38 columns).标准球状星团星表:坐标、距离、测光、[Fe/H]、E(B−V)、视向速度、结构、弛豫时间、中心密度(38 列)。
147 clusters · Harris W.E. 1996, AJ, 112, 1487
Vasiliev & Baumgardt 2021
VizieR J/MNRAS/505/5978
Precise Gaia EDR3 proper motions + parallaxes (→ distances); the most accurate GC astrometry to date.Gaia EDR3 精密自行 + 视差(→ 距离);迄今最精确的球状星团天体测量。
170 clusters · MNRAS, 505, 5978
Baumgardt & Hilker 2018
VizieR J/MNRAS/478/1520
Dynamical parameters: masses, mass-to-light ratios, half-light radii, relaxation times, escape velocities, central velocity dispersions.动力学参数:质量、质光比、半光半径、弛豫时间、逃逸速度、中心速度弥散。
112 clusters · MNRAS, 478, 1520
Bica et al. 2019
VizieR J/AJ/157/12
A census of Milky Way star clusters and candidates (including newly discovered globular-cluster candidates).银河系星团及候选体的普查(含新发现的球状星团候选体)。
10978 objects · AJ, 157, 12
galstreams — Mateu 2023
github.com/cmateu/galstreams
The most comprehensive library of Milky Way stellar-stream 6-D tracks: GD-1, Pal 5, Orphan-Chenab, Cetus, ATLAS-Aliqa Uma, and more.最全面的银河系恒星流 6 维轨迹库:GD-1、Pal 5、Orphan-Chenab、Cetus、ATLAS-Aliqa Uma 等。
124 streams · MNRAS, 520, 5225
Galaxy model — Reid+2019 / Vallée 2017 / Wegg+2015
spiral arms & bar旋臂与棒
Log-spiral arm parameters (Reid 2019 VLBI parallaxes; Vallée 2017 review); central-bar half-length and orientation (Wegg 2015).对数螺旋臂参数(Reid 2019 VLBI 视差;Vallée 2017 综述);中央棒半长与取向(Wegg 2015)。
ApJ 885,131 · ApJ 834,151 · MNRAS 450,4050

Methods & Models方法与模型

Spiral arms / bar / bulge旋臂 / 棒 / 核球 science-parameterized particles科学参数化粒子

  • 4 major arms (Scutum-Centaurus, Sagittarius-Carina, Perseus, Norma-Outer) + Outer arm + Local Arm (Orion Spur)4 条主旋臂(盾牌–半人马、人马–船底、英仙、矩尺–外臂)+ 外臂 + 本地臂(猎户支臂)
  • Log-spiral model, pitch angles 8–16° (Reid 2019 / Vallée 2017)对数螺旋模型,螺距角 8–16°(Reid 2019 / Vallée 2017)
  • Central bar: half-length 5 kpc, tilted 28° (Wegg 2015) + boxy/peanut bulge中央棒:半长 5 kpc,倾角 28°(Wegg 2015)+ 箱形/花生状核球
  • The Sun sits on the Local Arm (Orion Spur)太阳位于本地臂(猎户支臂)上
R(β) = R_ref · exp( −(β − β_ref) · tan ψ )

Orbit integration轨道积分 135 smooth orbits135 条平滑轨道

  • Potential MWPotential2014 (Hernquist bulge + Miyamoto-Nagai disk + NFW halo)势场 MWPotential2014(Hernquist 核球 + Miyamoto-Nagai 盘 + NFW 暗晕)
  • Calibrated to vc(R☉) = 238 km/s; self-implemented IAU 1958 transform标定至 vc(R☉) = 238 km/s;自实现 IAU 1958 坐标变换
  • scipy DOP853 (8th-order Runge-Kutta), back-integrated 3 Gyr, rtol=1e-7scipy DOP853(8 阶 Runge-Kutta),反向积分 3 Gyr,rtol=1e-7
  • Outputs R_peri / R_apo / eccentricity / z_max / prograde-vs-retrograde输出 R_peri / R_apo / 偏心率 / z_max / 顺行–逆行
R☉ = 8.275 kpc v☉ = (11.1, 251.24, 7.25) km/s 3 Gyr back-integration

Data-Accuracy Validation数据精度校验 spot checks against the literature与文献逐项核对

Check核对项Result结果Status状态
Row counts vs VizieR行数 vs VizieR147 / 170 / 112 / 10978✓ match
Coordinate consistency (Harris vs Gaia EDR3)坐标一致性(Harris vs Gaia EDR3)median offset 0.048′ (≈3″)✓ reliable
Circular velocity at the Sun太阳处圆周速度238.0 km/s✓ MWPotential2014
47 Tuc Galactic coordinates47 Tuc 银道坐标l=305.89°, b=−44.89°✓ lit. 305.90, −44.89
Orbit start vs catalog position轨道起点 vs 星表位置offset ≈ 0.02 kpc✓ same frame
Online 3D app (headless test)在线 3D 应用(无头测试)176 clusters / 124 streams / 0 JS errors / 120 fps✓ pass

Reproduce & Cite复现与引用

The pipeline is fully scripted and the catalog ships with the repo — rerun every step from raw VizieR tables to web data. If the atlas supports your work, cite the project and acknowledge the underlying surveys listed under Data Foundation. 整条数据管线均有脚本、星表随仓库发布——从 VizieR 原始表到网页数据可一步步复现。若本图谱对你的工作有帮助,请引用本项目,并向 数据基础 中列出的底层巡天数据致谢。

# Clone the repo
git clone git@github.com:jianxing-chen/globular-cluster-atlas.git
cd globular-cluster-atlas

# Open the 3D app (zero install)
open viz/index.html        # macOS
# start viz\index.html   # Windows
# xdg-open viz/index.html# Linux
# Re-run the data pipeline (optional)
cd scripts
python3 download_catalogs.py   # 1 fetch from VizieR
python3 parse_and_validate.py  # 2 parse + validate
python3 build_master.py        # 3 merge master catalog
python3 integrate_orbits.py    # 4 orbit integration
python3 process_streams.py     # 5 stellar streams
python3 make_figures.py        # 6 static figures
python3 export_viz_data.py     # 7 bundle web data
Dependencies: numpy · pandas · matplotlib · scipy (orbits/figures are self-implemented; no astropy/galpy needed)依赖:numpy · pandas · matplotlib · scipy(轨道与绘图均自实现,无需 astropy/galpy)

Cite the project引用本项目 APA style

# APA
Chen, J. (2026). Milky Way Globular Cluster Atlas [Computer software].
Retrieved from https://github.com/jianxing-chen/globular-cluster-atlas

BibTeXBibTeX LaTeX / Overleaf

# BibTeX
@software{chen2026gcatlas,
  author = {Chen, Jianxing},
  title  = {Milky Way Globular Cluster Atlas},
  year   = {2026},
  url    = {https://github.com/jianxing-chen/globular-cluster-atlas},
  note   = {Interactive 3D explorer + APJ-style figure workbench}
}

Acknowledgement template致谢模板

# Suggested acknowledgement text
This work made use of the Milky Way Globular Cluster Atlas (Chen 2026,
https://github.com/jianxing-chen/globular-cluster-atlas). The atlas aggregates
catalogues from CDS VizieR (Harris 1996/2010; Vasiliev & Baumgardt 2021;
Baumgardt & Hilker 2018; Bica et al. 2019) and stellar-stream tracks from the
galstreams library (Mateu 2023). This work has made use of data from the
European Space Agency (ESA) mission Gaia, processed by the Gaia Data
Processing and Analysis Consortium (DPAC).
The project is released under the MIT License; the aggregated data remain the property of their respective authors and institutions (see Data Foundation).本项目以 MIT 许可证 发布;聚合数据归各自作者与机构所有(见 数据基础)。