Luminosity effect of O i 7771–5 triplet and atmospheric microturbulence in evolved A-, F-, and G-type stars-Reference-Cited by-同舟云学术

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Luminosity effect of O i 7771–5 triplet and atmospheric microturbulence in evolved A-, F-, and G-type stars

Published:2018-01-01 Issue:1 Volume:70 Page:
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Takeda Yoichi¹²,Jeong Gwanghui³,Han Inwoo⁴³

Affiliation:

1. National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

2. SOKENDAI, The Graduate University for Advanced Studies, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

3. Korea University of Science and Technology, 217, Gajeong-ro, Yuseong-gu, Daejeon 34113, Korea

4. Korea Astronomy and Space Science Institute, 776, Daedeokdae-Ro, Youseong-Gu, Daejeon 34055, Korea

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/70/1/8/24001221/psx155.pdf

Reference41 articles.

1. The effective temperature scale of giant stars (F0–K5)

2. A new discussion on the $M_v$ – W(O I 7774 Å) relationship for F–G stars in the light of high-resolution data⋆

3. Calibrations of M[SUB]v[/SUB], (FE/H), and log G for yellow supergiant stars from O I 7774 and uvby-beta data

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1. Multiepoch Optical Spectroscopy of the Post-AGB Star HD 161796;The Astrophysical Journal;2022-03-01

2. High-Resolution Optical Spectroscopy of the Post-AGB Supergiant V340 Ser ($${\mathbf{=}}$$IRAS 17279$$\mathbf{-}$$1119);Astronomy Letters;2020-08

3. Do Hertzsprung‐gap stars show any chemical anomaly?;Astronomische Nachrichten;2019-06

4. Compositional differences between the component stars of eclipsing close binary systems showing chemical peculiarities;Monthly Notices of the Royal Astronomical Society;2019-02-14

5. Spectroscopic Determination of Capella’s Photospheric Abundances: Possible Influence of Stellar Activity;The Astrophysical Journal;2018-07-23

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