Abundance trends in kinematical groups of the Milky Way's disk

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

13 pages, accepted in A&A, Catalogue of data available at http://www.obs.u-bordeaux1.fr/m2a/soubiran/abundance-kinematics.html

Scientific paper

10.1051/0004-6361:20042390

We have compiled a large catalogue of metallicities and abundance ratios from the literature in order to investigate abundance trends of several alpha and iron peak elements in the thin disk and the thick disk of the Galaxy. The catalogue includes 743 stars with abundances of Fe, O, Mg, Ca, Ti, Si, Na, Ni and Al in the metallicity range -1.30 < [Fe/H] < +0.50. We have checked that systematic differences between abundances measured in the different studies were lower than random errors before combining them. Accurate distances and proper motions from Hipparcos, and radial velocities from several sources have been retreived for 639 stars and their velocities (U,V,W) and galactic orbits have been computed. Ages of 322 stars have been estimated with the Bayesian method of isochrone fitting developped by Pont & Eyer (2004). Two samples kinematically representative of the thin and thick disks have been selected, taking into account the Hercules stream which is intermediate in kinematics, but with a probable dynamical origin. [Abridged...]

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Abundance trends in kinematical groups of the Milky Way's disk 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 Abundance trends in kinematical groups of the Milky Way's disk, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Abundance trends in kinematical groups of the Milky Way's disk will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-135501

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.