English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

The statistical analysis of gathered of astronomical objects (such as opencluster) are excellent tools to compute its parameters and to constrain thetheory of its evolution. Here, we are represented detailed structural andmembership analysis of an open cluster NGC 1960 through various statisticalformulas and approaches. King empirical methods provide the information aboutthe cluster extent as 5.2 +/- 0.4 pc. The exact identification of members ofcluster is needed to precise estimation of its age, reddening, metallicityetc., therefore, to identify most probable members (MPMs), we adopted thecombined approach of various statistical methods (kinematic, photometric andstatistical) and 712 members are satisfied needed criteria of MPMs. The basicphysical parameters of the cluster such as E(B-V)=0.23+/-0.02 mag,E(V-K)=1.05+/-0.03mag, log(Age)=7.35+/-0.05, and (m-M)=11.35+/-0.10 mag areobtained using the color-color and color-magnitude diagrams. NGC 1960 is foundto be located at a distance of 1.34 +/- 0.03 kpc. Using the archival propermotion catalogues, we estimate mean proper motions of NGC 1960 as 0.83+/-0.26mas yr-1 and -6.55+/-0.23 mas yr-1 in the direction of RA and DEC,respectively.

Statistical analysis for precise estimation of structural properties of NGC 1960