Photocentric and Photometric Variability of Red Supergiant Stars

被引：0

作者：

Chiavassa, A. ^{[1
]}

Pasquato, E. ^{[1
]}

Jorissen, A. ^{[1
]}

Sacuto, S. ^{[2
]}

Babusiaux, C. ^{[3
]}

Freytag, B. ^{[4
,5
,6
,7
]}

Ludwig, H. -G. ^{[8
]}

Cruzalebes, P. ^{[9
]}

Rabbia, Y. ^{[9
]}

Spang, A. ^{[9
]}

Chesneau, O. ^{[9
]}

机构：

[1] Univ Libre Bruxelles, Inst Astron & Astrophys, Brussels, Belgium

[2] Univ Vienna, A-1010 Vienna, Austria

[3] Observ Paris, CNRS, GEPI, Paris, France

[4] Univ Lyon 1, F-69622 Villeurbanne, France

[5] Ecole Normale Super Lyon, Lyon, France

[6] Ctr Rech Astro Phys Lyon, CNRS, Saint Genis Laval, France

[7] Osserv Astron Capodimonte, Inst Nazl Astrofis, Naples, Italy

[8] Heidelberg Univ, Zentrum Astronomie, D-69115 Heidelberg, Germany

[9] Univ Nice Sophia Antipolis, Observat Cote Azur, CNRS, Fizeau Lab, Grasse, France

来源：

WHY GALAXIES CARE ABOUT AGB STARS II: SHINING EXAMPLES AND COMMON INHABITANTS | 2011年 / 445卷

关键词：

CONVECTION; BETELGEUSE;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Red supergiant stars are characterized by large convection-related surface structures that cause surface inhomogeneities and shock waves. We explore the impact of granulation on photocentric and photometric variability using 3D simulations of convection with CO5BOLD and the post-processing radiative transfer code OpTim3D to compute spectra and intensity maps in the Gaia G band (325 - 1030 nm).

引用

页码：169 / +

页数：2

共 5 条

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[3]

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[4]

2-H

[5]

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