On the Spectroscopic Determination of Atmospheric Parameters and O/Fe Abundances of RR Lyrae Stars

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概要

• 論文の詳細を見る
• 2006-04-25

著者

• TAKEDA Yoichi

  National Astronomical Observatory of Japan

• AOKI Wako

  National Astronomical Observatory of Japan

• Shi Jian-rong

  National Astronomical Observatories Chinese Academy Of Sciences

• Zhao Gang

  Fujitsu Kansai-chubu Net-tech Limited

• Zhao Gang

  National Astronomical Observatories Chinese Acad. Of Sci. Beijing Chn

• HONDA Satoshi

  National Research Institute of Fisheries Science, Fisheries Research Agency

• Honda Satoshi

  National Astronomical Observatory

• TAKADA HIDAI

  Liberal Arts Education Center, Tokai University

• Aoki W

  National Astronomical Observatory Of Japan Tokyo

• Aoki Wako

  National Astronomical Observatory

• Honda Satoshi

  Gunma Astronomical Observatory Gunma

• Chen Yu-qin

  National Astronomical Observatories Chinese Academy Of Sciences

• Yokoo Takeo

  Astronomical Institute Osaka Kyoiku University

• Takada Hidai

  Liberal Arts Education Center Tokai University

• Takeda Y

  The Graduate University For Advanced Studies

• Takeda Y

  Komazawa University

• Takeda Y

  Fracture Research Institute Graduate School Of Engineering Tohoku University

• Takeda Yoichi

  National Astronomical Observatory

• HONDA Satoshi

  Kwasan Observatory, Graduate School of Science, Kyoto University

• Honda Satoshi

  Kwasan Observatory Graduate School Of Science Kyoto University

• Honda Satoshi

  Kwasan Observatory Kyoto University

関連論文

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• Spectroscopic Observations of the WZ Sge-Type Dwarf Nova GW Librae during its 2007 Superoutburst
• Current Performance and On-Going Improvements of the 8.2m Subaru Telescope
• Substellar Companions to Evolved Intermediate-Mass Stars : HD 145457 and HD 180314
• Spin-Orbit Alignment of the TrES-4 Transiting Planetary System and Possible Additional Radial-Velocity Variation
• Spectral Evolution of the GRB 030329 Afterglow : Detection of the Supernova Nebular Phase Emissions
• Chemical Abundances of Outer Halo Stars in the Milky Way
• A SEARCH FOR EXOSPHERIC COMPONENTS OF THE EXTRASOLAR PLANET HD209458b WITH SUBARU HDS(Extrasolar Planetary Systems, International Symposium on Origins of Life and Astrobiology)
• Subaru HDS Transmission Spectroscopy of the Transiting Extrasolar Planet HD 209458b
• A Search for Hα Absorption in the Exosphere of the Transiting Extrasolar Planet HD 209458b
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• Iodine-Cell Spectroscopy at Okayama Astrophysical Observatory : First Results
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• Type-Ia Supernova SN 1995D in NGC 2962 : Optical V, R, and I Band Photometry and Spectra
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• Spectroscopic Determination of Stellar Atmospheric Parameters : Application to Mid-F through Early-K Dwarfs and Subgiants
• Abundance Analyses of 12 Parent Stars of Extrasolar Planets Observed with the SUBARU/HDS
• First Determination of the Actinide Thorium Abundance for a Red Giant of the Ursa Minor Dwarf Galaxy
• Metallicities in Four Planet-Harbouring K-Type Giants : HD 47536, HD 59686, HD 137759, and HD 219449
• Subaru/HDS Abundances in Three Giant Stars in the Ursa Minor Dwarf Spheroidal Galaxy
• Metallic Abundances in the Planet-Harboring G Type Star HD 217107
• Beryllium abundances of solar-analog stars
• Oxygen and Nitrogen Abundances in Hyades F Type Dwarfs
• The Short-Period Cepheid SU Cassiopeiae : Spectroscopic Diagnosis of its Rotation and Atmospheric Turbulence
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• High-Dispersion Spectroscopic Study of Solar Twins : HIP 56948, HIP 79672, and HIP 100963
• Stellar Parameters and Elemental Abundances of Late-G Giants
• Abundances of Volatile Elements in Post-AGB Candidates
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• Precise Differential Analysis of Stellar Metallicities : Application to Solar Analogs Including 16 Cyg A and B
• Photospheric CNO Abundances of Solar-Type Stars
• Lithium Abundances of F-, G-, and K-Type Stars : Profile-Fitting Analysis of the Li I 6708 Doublet
• Non-LTE Line-Formation and Abundances of Sulfur and Zinc in F, G, and K Stars
• Near-Infrared Spectra of 29 Carbon Stars : Simple Estimates of Effective Temperature
• Multiagent Cooperating Learning Methods by Indirect Media Communication
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• On the Abundance of Potassium in Metal-Poor Stars
• α Element Abundances in Mildly Metal-Poor Stars
• Convergence of the Q-ae Learning on Deterministic MDPs and Its Efficiency on the Stochastic Environment
• RTP-Q: A Reinforcement Learning System with Time Constraints Exploration Planning for Accelerating the Learning Rate
• Q-ee Learning : A Novel Q-Learning Method with Exploitation and Exploration
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• Spectroscopic Determination of Atmospheric Parameters of Solar-Type Stars: Description of the Method and Application to the Sun
• Abundance Analyses of 12 Parent Stars of Extrasolar Planets Observed with the SUBARU/HDS (Special Feature: Resent Results from the Subaru Telescope)
• Oxygen 6158-8 Å Triplet in Chemically Peculiar Stars of the Upper Main Sequence: Do HgMn Stars Show an Oxygen Anomaly?
• 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
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• Collecting duct carcinoma of the kidney : a case report
• Oxygen and Neon Abundances of B-Type Stars in Comparison with the Sun
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• Chromospheres in Metal-Poor Stars Evidenced from the HeI 10830 A Line
• Exploring the [S/Fe] Behavior of Metal-Poor Stars with the SI 1.046μm Lines
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• An Abundance Analysis of the Primary Star of the Peculiar Eclipsing Binary ε Aurigae out of the Eclipsing Phase
• The Rossiter-McLaughlin Effect of the Transiting Exoplanet XO-4b
• Drastic Spectroscopic Variability of the Be/X-Ray Binary Ariel 0535+262/V725 Tau during and after the 2009 Giant Outburst
• Further Observations of the Tilted Planet XO-3 : A New Determination of Spin-Orbit Misalignment, and Limits on Differential Rotation
• XO-2b : a Prograde Planet with Negligible Eccentricity and an Additional Radial Velocity Variation
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• Low-Resolution Spectroscopy of Hot Post-AGB Candidates II. LS, LSS, LSE Stars and Additional IRAS Sources
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• Behavior of [S/Fe] in Very Metal-Poor Stars from the SI 1.046μm Lines Revisited
• Electron Impact Excitation of N-like Ca XIV

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