Alpha Per cluster low-mass members. I. (Prosser+, 1998)

Details Alpha Per cluster low-mass members. I. (Prosser+, 1998) Alpha Per cluster low-mass members. I. (Prosser+, 1998)

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ycatp001031901p&link_type=abstract

VizieR On-line Data Catalog: J/other/AN/319.201. Originally published in: 1998AN....319..201P

Other

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

Scientific paper

Following the work of Randich et al. (1996A&A...305..785R) involving a ROSAT raster scan survey of the α Persei open cluster, we present here the results of a photometric/spectroscopic program examining the possible optical counterparts to a group of 73 X-ray sources in the raster survey which were not matched to catalogued stars. Of the 73 sources investigated, ~40 have an optical counterpart with photometry acceptable for cluster membership and ~20 of these also have radial velocities consistent with membership. We discuss the X-ray properties of these potential new members and why they may not have been identified in earlier membership surveys of this cluster. (3 data files).

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