Article
Open Access
Pulsation of IU Per from the Ground-based and ‘Integral’ Photometry
-
E. Kundra
,
L. Hric
Published/Copyright:
February 18, 2017
Received: 2012-10-17
Revised: 2013-4-4
Accepted: 2013-4-16
Published Online: 2017-2-18
Published in Print: 2013-6-1
© 2013 E. Kundra et al., published by De Gruyter Open
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
Keywords for this article
stars: binaries: eclipsing;
stars: oscillations;
stars: variables: δ Scuti;
stars: individual (IU Per)
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
