XMM observations of NGC 2547 (Jeffries+, 2006)

Details XMM observations of NGC 2547 (Jeffries+, 2006) XMM observations of NGC 2547 (Jeffries+, 2006)

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..73670781j&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/367/781. Originally published in: 2006MNRAS.367..781J

Physics

Clusters: Open, X-Ray Sources, Photometry: Ubvri

Scientific paper

The following tables describe the results of a survey for X-ray (0.3-3 keV) sources in the young (30Myr) NGC 2547 open cluster using the XMM-Newton EPIC instrument.
Table 1 lists the details of X-ray sources which are correlated with optical cluster members.
Table 2 catalogues the cross-identifications with optical catalogues for the sources in Table 1 and derives their X-ray luminosities and X-ray to bolometric flux ratios.
Table 3 lists the X-ray properties of sources which are uncorrelated with cluster members.
Table 7 lists the correlations between cluster members detected by XMM-Newton and those detected 7 years earlier by the ROSAT HRI instrument, along with the X-ray luminosities and flux ratios as determined by the HRI.
(4 data files).

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