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19 April 2024
 
  » arxiv » astro-ph/0205300

 Article overview


Rotation and activity in the solar-metallicity open cluster NGC2516
Donald M. Terndrup ; Marc Pinsonneault ; Robin D. Jeffries ; Alison Ford ; John R. Stauffer ; Alison Sills ;
Date 17 May 2002
Subject astro-ph
Affiliation Ohio State, Keele University, IPAC/Caltech, McMaster University
AbstractWe report new measures of radial velocities and rotation rates (v sin i) for 51 F and early-G stars in the open cluster NGC2516, and combine these with previously published data. From high signal-to-noise spectra of two stars, we show that NGC2516 has a relative iron abundance with respect to the Pleiades of delta([Fe/H])= +0.04 +/- 0.07 at the canonical reddening of E(B - V) = 0.12, in contrast to previous photometric studies that placed the cluster 0.2 to 0.4 dex below solar. We construct a color-magnitude diagram based on radial velocity members, and explore the sensitivity of photometric determinations of the metallicity and distance to assumed values of the reddening. For a metal abundance near solar, the Hipparcos distance to NGC2516 is probably underestimated. Finally, we show that the distribution of rotation rates and X-ray emission does not differ greatly from that of the Pleiades, when allowance is made for the somewhat older age of NGC2516.
Source arXiv, astro-ph/0205300
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