Berkeley 76: An intermediate age open star cluster in Gaia Era-Reference-Cited by-同舟云学术

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Berkeley 76: An intermediate age open star cluster in Gaia Era

Published:2024-07 Issue: Volume:109 Page:102205
ISSN:1384-1076
Container-title:New Astronomy
language:en
Short-container-title:New Astronomy

Author:

Bisht Deepak^ORCID,Bisht D.^ORCID,Raj A.,Rangwal Geeta,Sariya Devesh P.,Manu Mehul

Publisher

Elsevier BV

Reference72 articles.

1. On open cluster physical parameters from 2MASS data;Alves;New Astron.,2012

2. Estimating distances from parallaxes;Bailer-Jones;Publ. Astron. Soc. Pac.,2015

3. Estimating distance from parallaxes. IV. Distances to 1.33 billion stars in Gaia data release 2;Bailer-Jones;Astron. J.,2018

4. Determination of proper motions and membership of the open clusters NGC 1817 and NGC 1807;Balaguer-Núñez;Astron. Astrophys. Suppl. Ser.,1998

5. Determination of proper motions and membership of the open clusters NGC 1817 and NGC 1807;Balaguer-Núnez;Astron. Astrophys. Suppl. Ser.,1998

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1. Utilizing Voronoi Tessellations to Determine Radial Density Profiles;The Astronomical Journal;2024-07-02

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