Oxygen Abundances in Late-B through F Supergiants
スポンサーリンク
概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 1998-12-01
著者
-
Takada-hidai Masahide
Research Institute Of Civilization Tokai University
-
TAKEDA Yoichi
Institute of Astronomy, The University of Tokyo
-
Takeda Yoichi
Institute Of Astronomy Faculty Of Science The University Of Tokyo
-
Takeda-Hidai Masahide
Research Institute of Civilization, Tokai University
関連論文
- Metallic Abundances in the Planet-Harboring G-Type Star HD 38529
- Type-Ia Supernova SN 1995D in NGC 2962 : Optical V, R, and I Band Photometry and Spectra
- Line-Profile Analysis of KI 7699 in the Sun and in Procyon
- An Abundance Study in the Hg-Mn Star 46 Aquilae (HD 186122) with the SUBARU/HDS^1
- Metallic Abundances in the Planet-Harboring G Type Star HD 217107
- Oxygen and Nitrogen Abundances in Hyades F Type Dwarfs
- The Short-Period Cepheid SU Cassiopeiae : Spectroscopic Diagnosis of its Rotation and Atmospheric Turbulence
- α Element Abundances in Mildly Metal-Poor Stars
- Oxygen 6158-8 Å Triplet in Chemically Peculiar Stars of the Upper Main Sequence: Do HgMn Stars Show an Oxygen Anomaly?
- Non-LTE Abundance Analyses of Nitrogen and Sulfur in Chemically Peculiar Stars of the Upper Main Sequence
- Profile Analysis of He I 6678 in Beta Orionis : Rotation, Macroturbulence, and He Abundance
- On the Abundances of Nitrogen and Sulfur in Late-B through F Supergiants Atmospheres
- Nuclear-to-Disk Rotation Curves of Galaxies in the Hα and[NII]Emission Lines
- Helium and Carbon Abundances in Late-B and Early-A Supergiants
- Oxygen Abundances in Late-B through F Supergiants
- Deneb's Light-Element Abundances Revisited
- Spectroscopic Study of C, N, O, and S Abundances in a Field Horizontal-Branch Star HD 161817
- Non-LTE Analysis of the Oxygen λλ 7771-5 Triplet in Mid-G through Early-K Giants
- Oxygen λ7771-5 Triplet in Hyades A-Type Stars : A Quest for the Key to the Am Phenomenon
- Oxygen-Line Formation in Population-II A-Type Stars
- Self-Consistent Multi-Parameter Fitting of Stellar Flux Spectra
- Analyses of Line Profiles in the Solar Flux Spectrum for Determining Rotation and Micro/Macro Turbulence
- Empirical Determinations of Atomic Parameters from the Profiles of Solar Oxygen and Sodium Lines