The structure of a recent nova shell as observed by ALMA

被引:13
作者
Diaz, Marcos P. [1 ]
Abraham, Zulema [1 ]
Ribeiro, Valerio A. R. M. [2 ,3 ,4 ]
Beaklini, Pedro P. B. [1 ]
Takeda, Larissa [1 ]
机构
[1] Univ Sao Paulo IAG USP, Inst Astron Geofis & Ciencias Atmosfer, Dept Astron, Rua Matao 1226, BR-05508900 Sao Paulo, Brazil
[2] Univ Aveiro, Dept Fis, CIDMA, Campus Univ Santiago, P-3810193 Aveiro, Portugal
[3] Inst Telecomunicacoes, Campus Univ Santiago, P-3810193 Aveiro, Portugal
[4] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, POB 9010, NL-6500 GL Nijmegen, Netherlands
基金
巴西圣保罗研究基金会;
关键词
stars:; novae; cataclysmic variables; stars: white dwarfs; radio continuum: stars; MASS EJECTION; MODELS; SHOCKS;
D O I
10.1093/mnrasl/sly121
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
High resolution ALMA observations of the recent (2.52 yr old) shell of Nova V5668 Sgr (2015) show a highly structured ionized gas distribution with small (10(15) cm) clumps. These are the smallest structures ever observed in the remnant of a stellar thermonuclear explosion. No extended contiguous emission could be found above the 2.5 sigma level in our data, while the peak hydrogen densities in the clumps reach 10(6) cm(-3). The millimetre continuum image suggests that large scale structures previously distinguished in other recent nova shells may result from the distribution of bright unresolved condensations.
引用
收藏
页码:L54 / L57
页数:4
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