On the near infrared variability of chemically peculiar stars
被引:0
作者:
Catalano, FA
论文数: 0引用数: 0
h-index: 0
机构:
Univ Catania, Ist Astron, I-95124 Catania, ItalyUniv Catania, Ist Astron, I-95124 Catania, Italy
Catalano, FA
[1
]
Leone, F
论文数: 0引用数: 0
h-index: 0
机构:
Univ Catania, Ist Astron, I-95124 Catania, ItalyUniv Catania, Ist Astron, I-95124 Catania, Italy
Leone, F
[1
]
机构:
[1] Univ Catania, Ist Astron, I-95124 Catania, Italy
来源:
PROCEEDINGS OF THE 26TH MEETING AND WORKSHOP OF THE EUROPEAN WORKING GROUP ON CP STARS
|
1998年
/
27卷
/
03期
关键词:
stars;
chemically peculiar;
variables;
other;
D O I:
暂无
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Same CP stars have recently been discovered by Catalano et al. (1991) to be variable also in the near infrared, although with smaller amplitudes than in the visible. Hence an observational campaign was started in which the infrared light variability of a number of CP2 and CP4 stars has been investigated at the ESO-La Silla Observatory in the bands J, H, and K. As a general result, infrared variations show the same behavior in all three filters but amplitudes are smaller than in the visible.