Abstract
The aim of the Round Table (RT) ”Problems in modelling stellar atmospheres“ was that of giving a panoramic view of the state of art on the atmospheric models used to predict observations of stars from T to A spectral type, the Sun included.
Keywords
Affiliated Institutions
Related Publications
Observed versus predicted stellar flux distributions of solar-type stars
I have compared the low-resolution spectrophotometric fluxes in the visible spectral region of F- and G-type MARCS 2008 model atmospheres to six spectrophotometric databases of ...
Spectral evolution of stellar populations using isochrone synthesis
view Abstract Citations (1953) References (74) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Spectral Evolution of Stellar Populations Using I...
The [ITAL]Forbidden[/ITAL] Abundance of Oxygen in the Sun
We reexamine closely the solar photospheric line at 6300 A, which is\nattributed to a forbidden line of neutral oxygen, and is widely used in\nanalyses of other late-type stars....
New Light on Stellar Abundance Analyses: Departures from LTE and Homogeneity
▪ Abstract The information on the chemical compositions of stars encoded in their spectra plays a central role in contemporary astrophysics. Stellar element abundances are, howe...
Chemical Abundances from Inversions of Stellar Spectra: Analysis of Solar‐Type Stars with Homogeneous and Static Model Atmospheres
Spectra of late-type stars are usually analyzed with static model atmospheres in local thermodynamic equilibrium (LTE) and a homogeneous plane-parallel or spherically symmetric ...
Publication Info
- Year
- 2003
- Type
- article
- Volume
- 210
- Pages
- 47-48
- Citations
- 524
- Access
- Closed
External Links
Social Impact
Social media, news, blog, policy document mentions
Citation Metrics
Cite This
Identifiers
- DOI
- 10.1017/s0074180900133248