Skip to main content
Journal Article

The super metal rich component of the galaxy

Astrophysics and Space Science (1999) 265(1-4) 341-344
DOI: 10.1007/978-94-011-4213-7_71
0Citations
Citations of this article
1Readers
Mendeley users who have this article in their library.
Get full text

Abstract

We present the results obtained by comparing mid-resolution stellar spectra of super metal rich candidates with synthetic spectra computed in the wavelength range 4850-5400 Å. Atmospheric parameters, derived by using the flux fitting method, are illustrated for a sample of representative stars. The final aim of the project is the definition of a fully consistent metallicity scale for SMR stars.

Cite

CITATION STYLE

APA

Malagnini, M. L., Morossi, C., Buzzoni, A., & Chavez, M. (1999). The super metal rich component of the galaxy. Astrophysics and Space Science, 265(1–4), 341–344. https://doi.org/10.1007/978-94-011-4213-7_71

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free