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P. Mondal

6 papers hereh-index 00 citations5 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author3
  • last author2

Across the 5 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
  • astro-ph.SR2
same name
  • P. Mondal — 28 papers, h 6
  • P. Mondal — 18 papers, h 14
  • P. Mondal — 12 papers, h 12
  • P. Mondal — 11 papers, h 9
  • P. Mondal — 10 papers, h 3
  • P. Mondal — 9 papers, h 22

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators
Showing astro-ph.GAShow all

4 papers · 1 filter

astro-ph.GA2026

Cluster Membership Probabilities: A Review of Methods and Gaia Applications

Tahereh Ramezani, Johana Balciráková, Prapti Mondal +3

Reliable stellar-cluster membership is essential for deriving cluster ages, distances, reddenings, metallicities, mass functions, dynamical parameters, and Galactic-structure trace…

astro-ph.GA2026

Tidal Tails of Galactic Open Clusters: A Review of Methods, Evidence, and Sources of Disagreement

Tahereh Ramezani, Prapti Mondal, Johana Balciráková +4

Tidal tails are a natural consequence of the dynamical evolution of open clusters in the Galactic tidal field, but their observational identification is intrinsically difficult bec…

astro-ph.GA2026

The different methods to calculate cluster membership probabilities

Tahereh Ramezani, Prapti Mondal, Katerina Neumannova +3

Reliable membership determination is a fundamental step in the study of star clusters. With the advent of Gaia astrometry, a wide range of statistical and machine-learning techni…

astro-ph.GA2026

Cluster characteristics of Galactic open clusters

K. Neumannová, J. Supíková, N. Faltová +4

Star clusters are perfectly suited for studying the formation, evolution, and dynamics of stars and their host galaxies. For this, we need to estimate total masses, radii and shape…

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