Abundances in Individual Stars of the Galactic Bulge

Details Abundances in Individual Stars of the Galactic Bulge Abundances in Individual Stars of the Galactic Bulge

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ap%26ss.265..319b&link_type=abstract

Astrophysics and Space Science, v. 265, Issue 1/4, p. 319-326 (1999).

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

Element ratios in two stars of NGC 6553 and one star in NGC 6528 reveal
that α-elements are enhanced relative to Fe. The metallicity
[Fe/H] ≈ -0.6, but taking into account the overabundances of
several elements, the overall metallicity is close to solar.

Affiliated with

Also associated with

No associations

Rating

Abundances in Individual Stars of the Galactic Bulge 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 Abundances in Individual Stars of the Galactic Bulge, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Abundances in Individual Stars of the Galactic Bulge will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1619011