uu.seUppsala University Publications
Change search
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf
Removal of the calcium underabundance in cool metal rich Galactic disk dwarfs
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2000 (English)In: ASTRONOMY AND ASTROPHYSICS, Vol. 358, no 1, L21-L23 p.Other (Other scientific)
Abstract [en]

An apparent Ca underabundance for cool metal rich disk dwarfs was derived by Feltzing & Gustafsson (1998). This was suggested to be a NLTE effect, following the prediction by Drake (1991). New NLTE calculations with MARCS atmospheres and opacities show th

Place, publisher, year, pages
SPRINGER VERLAG , 2000. Vol. 358, no 1, L21-L23 p.
Keyword [en]
atomic data; stars : abundances; stars : late-type; NEUTRAL CALCIUM; UVBY PHOTOMETRY; STARS BRIGHTER; HYDROGEN; TRANSITIONS
Identifiers
URN: urn:nbn:se:uu:diva-36665OAI: oai:DiVA.org:uu-36665DiVA: diva2:64564
Note
Addresses: Thoren P, Univ Uppsala, Astron Observ, Box 515, S-75120 Uppsala, Sweden. Univ Uppsala, Astron Observ, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17

Open Access in DiVA

No full text

By organisation
Department of Astronomy and Space Physics

Search outside of DiVA

GoogleGoogle Scholar

urn-nbn

Altmetric score

urn-nbn
Total: 354 hits
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf