Oxygen line formation in 3D hydrodynamical model atmospheres

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Invited talk presented at IAU General Assembly Joint Discussion 8 "Oxygen abundances in old stars and implications for nucleos

Scientific paper

The formation of [O I], O I and OH lines in metal-poor stars has been studied by means of 3D hydrodynamical model atmospheres. For O I detailed 3D non-LTE calculations have been performed. While the influence of 3D model atmospheres is minor for [O I] and O I lines, the very low temperatures encountered at low metallicities have a drastic impact on the OH lines. As a result, the derived O abundances are found to be systematically overestimated in 1D analyses, casting doubts on the recent claims for a monotonic increase in [O/Fe] towards lower metallicities.

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

Oxygen line formation in 3D hydrodynamical model atmospheres 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 Oxygen line formation in 3D hydrodynamical model atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Oxygen line formation in 3D hydrodynamical model atmospheres will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-453566

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