Skip to main content

The question of the abundance of metals in stars with planets

Buy Article:

$59.35 plus tax (Refund Policy)

Abstract:

The metal-poor stars with planets were compared with the metal-rich stars also with planets. The high [Fe]/[H] values obtained from the spectroscopic analysis for most stars with planets can be consequence of the fact that the models used are inadequate for real stellar atmospheres.

Keywords: Evolution of stars; Late-type stars; Metal abundances; Stars

Document Type: Research Article

DOI: http://dx.doi.org/10.1080/10556790500487031

Affiliations: Fesenkov Astrophysical Institute, Almaty, 050020, Kazakhstan

Publication date: August 1, 2005

More about this publication?
tandf/gaat/2005/00000024/00000004/art00014
dcterms_title,dcterms_description,pub_keyword
6
5
20
40
5

Access Key

Free Content
Free content
New Content
New content
Open Access Content
Open access content
Subscribed Content
Subscribed content
Free Trial Content
Free trial content
Cookie Policy
X
Cookie Policy
ingentaconnect website makes use of cookies so as to keep track of data that you have filled in. I am Happy with this Find out more