6533b883fe1ef96bd12dbe89

RESEARCH PRODUCT

XMM observations of NGC 2516 stars

A. MarinoG. MicelaI. PillitteriG. Peres

subject

Astrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLate type starsX-ray sourcesstellar astronomyOptical astronomyCosmologyOpen star clustersPhotometryobservational astronomyX ray sourcesAstrophysics::Solar and Stellar AstrophysicsWide-band photometryNatural SciencesLate-type starsAstrophysics::Galaxy AstrophysicsInfrared photometryWide band photometry

description

We present the characteristics of the X-ray variability of stars in the cluster NGC 2516 as derived from XMM-Newton/EPIC/pn data. The X-ray variations on short (hours), medium (months), and long (years) time scales have been explored. We detected 303 distinct X-ray sources by analysing six EPIC/pn observations; 194 of them are members of the cluster. Stars of all spectral types, from the early-types to the late-M dwarfs, were detected. Cone search capability for table J/A+A/456/977/table2 (X-ray and optical properties of NGC 2516 members in the XMM-Newton/EPIC/pn observations having more than 25 counts.)

10.26093/cds/vizier.34560977https://doi.org/http://doi.org/10.26093/cds/vizier.34560977