Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2011-01-17
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
28 pages, 6 figures, accepted for publication in AJ
Scientific paper
We present the chromospheric activity (CA) levels, metallicities and full space motions for 41 F, G, K and M dwarf stars in 36 wide binary systems. Thirty-one of the binaries, contain a white dwarf component. In such binaries the total age can be estimated by adding the cooling age of the white dwarf to an estimate of the progenitor's main sequence lifetime. To better understand how CA correlates to stellar age, 14 cluster member stars were also observed. Our observations demonstrate for the first time that in general CA decays with age from 50 Myr to at least 8 Gyr for stars with 1.0 < V-I < 2.4. However, little change occurs in CA level for stars with V-I < 1.0 between 1 Gyr and 5 Gyr, consistent with the results of Pace et al. (2009). Our sample also exhibits a negative correlation between stellar age and metallicity, a positive correlation between stellar age and W space velocity component and the W velocity dispersion increases with age. Finally, the population membership of these wide binaries is examined based upon their U, V, W kinematics, metallicity and CA. We conclude that wide binaries are similar to field and cluster stars in these respects. More importantly, they span a much more continuous range in age and metallicity than is afforded by nearby clusters.
Chen Yu-Qi
Oswalt Terry D.
Rudkin Merissa
Zhao Gang
Zhao Ji-Kuen
No associations
LandOfFree
The Chromospheric Activity, Age, Metallicty and Space Motions of 36 Wide Binaries does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Chromospheric Activity, Age, Metallicty and Space Motions of 36 Wide Binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Chromospheric Activity, Age, Metallicty and Space Motions of 36 Wide Binaries will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-286545