Fe i Lines in 0.91–1.33 μm Spectra of Red Giants for Measuring the Microturbulence and Metallicities-Reference-Cited by-同舟云学术

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Fe i Lines in 0.91–1.33 μm Spectra of Red Giants for Measuring the Microturbulence and Metallicities

Published:2019-04-23 Issue:2 Volume:875 Page:129
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Kondo Sohei,Fukue Kei,Matsunaga Noriyuki,Ikeda Yuji^ORCID,Taniguchi Daisuke,Kobayashi Naoto,Sameshima Hiroaki^ORCID,Hamano Satoshi,Arai Akira,Kawakita Hideyo,Yasui Chikako,Izumi Natsuko^ORCID,Mizumoto Misaki^ORCID,Otsubo Shogo,Takenaka Keiichi,Watase Ayaka,Asano Akira,Yoshikawa Tomohiro,Tsujimoto Takuji^ORCID

Funder

Supported Programs for the Strategic Research Foundation at Private Universities form MEXT of Japan

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab0ec4/pdf

Reference69 articles.

1. Abundances of the elements: Meteoritic and solar

2. The surface gravity of Arcturus from MgH lines, strong metal lines and the ionization equilibrium of iron

3. SP_Ace: a new code to derive stellar parameters and elemental abundances

4. Chemical composition of semi-regular variable giants. III.

5. High-resolution CCD spectra of stars in globular clusters. VII - Abundances of 16 elements in 47 Tuc, M4, and M22

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