NOVA CYGNI 1992 - SPECTRAL DEVELOPMENT IN THE NEAR-INFRARED AT MAXIMUM LIGHT

被引：7

作者：

ANDRILLAT, Y

HOUZIAUX, L

机构：

[1] UNIV LIEGE MON HAINAUT,INST MATH,IS AVE TILLEULS,B-4000 LIEGE,BELGIUM

[2] UNIV MONTPELLIER 2,ASTRON LAB,F-34095 MONTPELLIER 5,FRANCE

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1993年 / 261卷 / 01期

关键词：

STARS; INDIVIDUAL; NOVA CYGNI 1992; NOVAE; CATACLYSMIC VARIABLES;

D O I：

10.1093/mnras/261.1.L1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Spectroscopic observations of Nova Cygni 1992 in the range 0.64-1.15 mum from 1992 February 22 to 24 show-a-strong increase of emission in the HI OI and NI lines, and the onset of the two absorption systems on February 23. There are indications of a strong overabundance of nitrogen.

引用

页码：L1 / L4

页数：4