A method for determining the radius of an open cluster from stellar proper motions-Reference-Cited by-同舟云学术

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A method for determining the radius of an open cluster from stellar proper motions

Published:2018-01-10 Issue:3 Volume:475 Page:4122-4132
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Sánchez Néstor¹,Alfaro Emilio J²,López-Martínez Fátima³

Affiliation:

1. Departamento de Física, Universidad de Murcia, E-30100 Murcia, Spain

2. Instituto de Astrofísica de Andalucía, CSIC, Glorieta de la Astronomía s/n, E-18008, Granada, Spain

3. Centro de Astrofísica da Universidade do Porto, Rua das Estrelas, P-4150-762 Porto, Portugal

Funder

FEDER

Fundación Séneca de la Región de Murcia

Ministerio de Economía y Competitividad

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/475/3/4122/23965872/sty088.pdf

Reference53 articles.

1. Looking for phase-space structures in star-forming regions: an MST-based methodology

2. Minimal spanning trees, filaments and galaxy clustering

3. Source clustering in the Hi-GAL survey determined using a minimum spanning tree method

4. Spatial dependence of 2MASS luminosity and mass functions in the old open cluster NGC 188

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1. Exploration of morphological coherence in open clusters with a “core-shell” structure;Astronomy & Astrophysics;2024-07

2. Visualizing the pulsar population using graph theory;Monthly Notices of the Royal Astronomical Society;2022-08-05

3. Study of the open cluster Alessi-Teutsch 9 (ASCC 10) using multiband photometry and Gaia EDR3;Astrophysics and Space Science;2021-09

4. A catalogue of open cluster radii determined from Gaia proper motions;Monthly Notices of the Royal Astronomical Society;2020-01

5. Clusters and mirages: cataloguing stellar aggregates in the Milky Way;Astronomy & Astrophysics;2020-01

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