Photometry in the Open Cluster IC 2602 and NGC 6475

Details Photometry in the Open Cluster IC 2602 and NGC 6475 Photometry in the Open Cluster IC 2602 and NGC 6475

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aj....112..649p&link_type=abstract

Astronomical Journal v.112, p.649

Astronomy and Astrophysics

Astronomy

25

Open Clusters And Associations: Ic 2602, Open Clusters And Associations: Ngc 6475, X-Rays: Stars

Scientific paper

CCD photometry has been obtained in the regions of the open clusters IC 2602 and NGC 6475 for the purpose of identifying likely optical counterparts to x-ray sources. Photometry has also been obtained for relatively bright stars in both clusters in order to improve upon previous photometry and to assess membership. In IC 2602, the new candidate members associated with x-ray sources include two visual binary systems with the secondary components being the lowest-mass candidate members identified to date. in NGC 6475, several possible optical counterparts to the strongest x-ray source in the field of the cluster have been given, though the true optical counterpart remains unknown.

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