NTT VI photometry in Terzan 5

B2FIND2026-04-11 收录

球状星团测光

天体物理学

数据链接：

https://b2find.eudat.eu/dataset/5c8826a6-d9f2-5806-804c-8bb230cbd514 数据链接链接失效反馈

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资源简介：

We study the metal-rich bulge globular cluster Terzan 5 by means of VI colour-magnitude diagrams, with images obtained under exceptional seeing conditions (0.34"-0.50")....

arXiv Astro-Ph (arXiv Astro Physics)

天体物理学

科学合作网络

Arxiv ASTRO-PH（Astro Physics）合作网络来自电子版 arXiv，涵盖了提交给 Astro Physics 类别的作者论文之间的科学合作。如果作者 i 与作者 j 共同撰写了一篇论文，则该图包含从 i 到 j 的无向边。如果论文由 k 个作者共同撰写，则会在 k 个节点上生成一个完全连接的（子）图。

OpenDataLab2026-07-12 更新130

Parkes observations for project P427 semester 2008OCTS

脉冲星

天体物理学

Timing the dozen pulsars discovered in P303 is ensuring high quality results: (a) the peculiarities (in position or projected acceleration) of all the 5 millisecond pulsars in NGC6752 suggested the pr

Research Data Australia110

Long-term project observations for project P1041 semester 2025APRS_02

天体物理学

脉冲星研究

Omega Cen is the largest globular cluster in the Milky Way. I contains at least 18 known MPSs, and there are solid hints for the presence of an even larger pulsar population. We propose a regular mont

DataCite Commons2025-05-22 更新80

Parkes observations for project P1021 semester 2022OCTS_02

天体物理学

脉冲星

We propose to observe PSR J1812-15 and PSR J1831-04, a pair of long spin-period binary pulsars which both show degrees of orbitally-dependent variability. Binary pulsars are valuable objects of scient

Research Data Australia110

Replication Data for: Viscous dissipation in the fluid core of the Moon

天体物理学

月球研究

codes to reproduce results and script to redo all figures of the paper.

DataONE2022-01-04 更新100