Effective temperatures of red supergiants estimated from line-depth ratios of iron lines in the YJ bands, 0.97-1.32 μm (vol 502, pg 4210, 2021)

被引：0

作者：

Taniguchi, Daisuke ^{[1
]}

Matsunaga, Noriyuki ^{[1
,2
]}

Jian, Mingjie ^{[1
]}

Kobayashi, Naoto ^{[2
,3
,4
]}

Fukue, Kei ^{[2
]}

Hamano, Satoshi ^{[2
,5
]}

Ikeda, Yuji ^{[2
,6
]}

Kawakita, Hideyo ^{[2
,7
]}

Kondo, Sohei ^{[2
]}

Otsubo, Shogo ^{[2
]}

Sameshima, Hiroaki ^{[3
]}

Takenaka, Keiichi ^{[8
]}

Yasui, Chikako ^{[9
]}

机构：

[1] Univ Tokyo, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan

[2] Kyoto Sangyo Univ, Koyama Astron Observ, Lab Infrared High Resolut Spect LiH, Kita Ku, Kyoto 6038555, Japan

[3] Univ Tokyo, Inst Astron, 2-21-1 Osawa, Mitaka, Tokyo 1810015, Japan

[4] Univ Tokyo, Kiso Observ, 10762-30 Mitake,Kiso Machi, Nagano 3970101, Japan

[5] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan

[6] Photocoding, Sakyo Ku, 460-102 Iwakura Nakamachi, Kyoto 6060025, Japan

[7] Kyoto Sangyo Univ, Fac Sci, Dept Astrophys & Atmospher Sci, Kita Ku, Kyoto 6038555, Japan

[8] Kyoto Sangyo Univ, Div Sci, Grad Sch, Kita Ku, Kyoto 6038555, Japan

[9] Natl Astron Observ Japan, Calif Off, 100 W Walnut St,Suite 300, Pasadena, CA 91124 USA

来源：

关键词：

errata; addenda; techniques: spectroscopic; stars: atmospheres; stars: fundamental parameters; stars: late-type; supergiants; infrared: stars;

D O I：

10.1093/mnras/stac686

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：2669 / 2670

页数：2

共 2 条