SiO maser movies

被引：27

作者：

Gray, MD

Humphreys, EML

机构：

[1] Univ Wales, Dept Phys & Astron, Cardiff CF24 3YB, S Glam, Wales

[2] Onsala Space Observ, S-43992 Onsala, Sweden

来源：

NEW ASTRONOMY | 2000年 / 5卷 / 03期

关键词：

masers; stars : AGB and post-AGB; circumstellar matter; radio lines : stars; stars : individual : TX cam;

D O I：

10.1016/S1384-1076(00)00020-8

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We show how the intensity and spatial distribution of silicon monoxide masers varies with time according to the parameters of a current model. The variation of the masers at 43 GHz in the v = 1 vibrational state is presented as an animation. Where possible, comparisons are drawn with a similar animation of the real Mira variable TX Cameleopardalis. (C) 2000 Elsevier Science B.V. All rights reserved.

引用

页码：155 / 162

页数：8

共 49 条

[1]

Barthes D, 1998, ASTRON ASTROPHYS, V333, P647

[2]

BEACH TE, 1990, THESIS IOWA STATE U

[3] Mode switching in the nearby Mira-like variable R Doradus [J].