The question of the abundance of metals in stars with planets

$61.20 plus tax (Refund Policy)

Buy Article:

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?
Related content

Share Content

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