Near-infrared photometry of the final helium shell flash object V4334 Sagittarii

被引:14
|
作者
Kamath, US [1 ]
Ashok, NM [1 ]
机构
[1] Phys Res Lab, Astron & Astrophys Div, Ahmedabad 380009, Gujarat, India
关键词
techniques : photometric; stars : AGB and post-AGB; circumstellar matter; stars : individual : V4334 Sgr; stars : peculiar; infrared : stars;
D O I
10.1046/j.1365-8711.1999.02142.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
JHK photometry of the final helium shell flash object V4334 Sagittarii undertaken during 1996-97 is presented in this paper. The data reveal the formation of circumstellar dust of temperature similar to 1800 K two years after outburst. Around 5 x 10(-10) M-circle dot of dust condensed at a distance of about 7R* from the star. The mass of V4334 Sgr is 0.8 M-circle dot and it had a radius of similar to 70 R-circle dot in 1997 April-May.
引用
收藏
页码:512 / 514
页数:3
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