X-ray detections in the σ Ori cluster (Caballero+, 2010)

Details X-ray detections in the σ Ori cluster (Caballero+, 2010) X-ray detections in the σ Ori cluster (Caballero+, 2010)

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35219045c&link_type=abstract

VizieR On-line Data Catalog: J/A+A/521/A45. Originally published in: 2010A&A...521A..45C

Computer Science

Clusters: Open, Stars: Early-Type, X-Ray Sources

Scientific paper

We used public HRC-I/Chandra data from a 97.6ks pointing towards the cluster centre and complemented them with X-ray data from IPC/Einstein, HRI/ROSAT, EPIC/XMM-Newton, and ACIS-S/Chandra together with optical and infrared photometry and spectroscopy from the literature and public catalogues. On our HRC-I/Chandra data, we measured count rates, estimated X-ray fluxes, and searched for short-term variability. We also looked for long-term variability by comparing with previous X-ray observations.
(3 data files).

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