From the 1 of 11 linked papers with an AI index.
14 papers
The white dwarf population of open clusters and their tidal tails. Tracers of contamination and stellar interactions
Vikrant V. Jadhav, Pavel Kroupa, David R. Miller +3
The study uses Gaia DR3 data to identify white dwarfs linked to open clusters and their tidal tails, evaluates contamination rates, and compares the observed white dwarf population…
Connecting Star Formation in the Milky Way and Nearby Galaxies -II. An Observationally Driven Analytical Model for Predicting Cloud-Scale Star Formation Rates
J. W. Zhou, Amelie Saintonge, Sami Dib +1
We construct a model by integrating observational constraints from the Milky Way and nearby galaxies to predict cloud-scale star formation rates (SFRs). In the model, we first esti…
Statistical study for binary star evolution in dense embedded clusters
Wenjie Wu, Pavel Kroupa, Vikrant V. Jadhav
Context: The dynamical evolution of binary populations in embedded star clusters shapes the statistical properties of binaries observed in the Galactic field. Accurately modelling…
Tidal Tails of Nearby Open Clusters. II. A Review of Simulated Properties and the Reliability of Observational Catalogues
Vikrant V. Jadhav, Dhanraj Risbud, Pavel Kroupa +1
Context: Recent studies using Gaia data have reported tidal tail detections for tens to hundreds of open clusters. However, a comprehensive assessment of the reliability & complete…
The most massive star clusters in molecular clouds: Insights from the integrated cloud-wide initial mass function (ICIMF) theory
J. W. Zhou, Pavel Kroupa, Sami Dib
The combination of the high-resolution ALMA, JWST and HST observations provides unprecedented insights into the connection between individual molecular clouds and their internal st…
Inversely synthesizing the core mass function of high-mass star-forming regions from the canonical initial mass function
J. W. Zhou, Pavel Kroupa, Sami Dib
Many studies have revealed that the core mass function (CMF) in high-mass star-forming regions is top-heavy. In this work, we start from the canonical initial mass function (IMF) t…