Metallic Abundances in the Planet-Harboring G-Type Star HD 38529

Details Metallic Abundances in the Planet-Harboring G-Type Star HD 38529 Metallic Abundances in the Planet-Harboring G-Type Star HD 38529

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001pasj...53..315s&link_type=abstract

Publications of the Astronomical Society of Japan, vol.53, no. 2, p. 315-320.

Astronomy and Astrophysics

Astronomy

9

Planetary Systems, Stars: Abundances, Stars: Individual (Hd 38529)

Scientific paper

The abundances of 16 elements (C through Y) in the recently detected planet-harboring G4 IV star HD 38529 are presented. A spectroscopic analysis was carried out differentially relative to the Sun. The adopted atmospheric parameters of the star are Teff = 5500 +/- 100 K,log g = 3.6 +/- 0.1, ξt = 1.0 +/- 0.3 km s-1, and [M/H] = +0.3. Iron is definitely overabundant with respect to the Sun, [Fe/H] = +0.40 +/- 0.06, and all other elements are also found to be enhanced. The enhancements of iron peak elements (Ti through Ni) are coincident with that of Fe within +/- 0.1 dex, while C and O are slightly less enhanced than Fe.

Affiliated with

Also associated with

No associations

Rating

Metallic Abundances in the Planet-Harboring G-Type Star HD 38529 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 Metallic Abundances in the Planet-Harboring G-Type Star HD 38529, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Metallic Abundances in the Planet-Harboring G-Type Star HD 38529 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-962308