Article
Open Access
A New High-Precision Correction Method of Temperature Distribution in Model Stellar Atmospheres
-
A. Sapar
,
R. Poolamäe
Published/Copyright:
February 18, 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
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- 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
Creative Commons
BY-NC-ND 3.0
Articles in the same Issue
- 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
