Artikel
Open Access
A New High-Precision Correction Method of Temperature Distribution in Model Stellar Atmospheres
-
A. Sapar
,
R. Poolamäe
Veröffentlicht/Copyright:
18. Februar 2017
Received: 2013-1-9
Accepted: 2013-3-27
Published Online: 2017-2-18
Published in Print: 2013-6-1
© 2013 A. Sapar et al., published by De Gruyter Open
Artikel in diesem Heft
- Peculiarities and Variations in the Optical Spectrum of the RV Tauri-type Star R Sct
- On the Spectrum of Extremely Metal-Poor Star HD 52961
- Pulsation of IU Per from the Ground-based and ‘Integral’ Photometry
- Further Investigation of the Effect of Galaxy Interactions on Star Formation
- Environmental Dependence of Different Colors for the Apparent Magnitude-Limited Main Galaxy Sample of the SDSS DR7
- A New High-Precision Correction Method of Temperature Distribution in Model Stellar Atmospheres
- New Methods in Modeling of Hot Stellar Atmospheres
Schlagwörter für diesen Artikel
stars: atmospheres;
stars: early-type;
stars: fundamental parameters
Creative Commons
BY-NC-ND 3.0
Artikel in diesem Heft
- Peculiarities and Variations in the Optical Spectrum of the RV Tauri-type Star R Sct
- On the Spectrum of Extremely Metal-Poor Star HD 52961
- Pulsation of IU Per from the Ground-based and ‘Integral’ Photometry
- Further Investigation of the Effect of Galaxy Interactions on Star Formation
- Environmental Dependence of Different Colors for the Apparent Magnitude-Limited Main Galaxy Sample of the SDSS DR7
- A New High-Precision Correction Method of Temperature Distribution in Model Stellar Atmospheres
- New Methods in Modeling of Hot Stellar Atmospheres
