Helium and Carbon Abundances in Late-B and Early-A Supergiants

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概要

• 論文の詳細を見る
• Astronomical Society of Japanの論文
• 2000-02-25

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

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

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