X-ray observations of IC348 in light of an updated cluster census
B.Stelzer, G.Micela, E.Flaccomio, S.Sciortino (INAF - Osservatorio, Astronomico di Palermo)
TL;DR
This paper re-analyzes Chandra X-ray data of the IC348 cluster in light of new optical and infrared observations that updated the cluster's census, aiming to improve understanding of low-mass star formation.
Contribution
It provides a revised analysis of X-ray observations incorporating recent multi-wavelength data, offering new insights into the cluster's stellar population.
Findings
Updated cluster census with new optical/infrared data
Refined X-ray source properties and membership
Enhanced understanding of low-mass star formation in IC348
Abstract
IC348 is an excellent laboratory for studies of low-mass star formation being nearby, compact and rich. A Chandra observation was carried out early in the satellite's lifetime. The extensive new data in optical and infrared wavelengths accumulated in subsequent years have changed the cluster census calling for a re-analysis of the X-ray data.
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