Fabry-Perot observations of HH 1/2

被引：0
作者：
Riera, A
Raga, AC
Reipurth, B
Amram, P
Boulesteix, J
Toledano, O
机构：
[1] Univ Politecn Catalunya, Dept Fis & Engn Nucl, E-08800 Vilanova I La Geltru, Spain
[2] Univ Barcelona, Dept Astron & Meteorol, E-08007 Barcelona, Spain
[3] Univ Nacl Autonoma Mexico, Inst Ciencias Nucl, Mexico City 04510, DF, Mexico
[4] Univ Hawaii, Inst Astron, Hilo, HI 96720 USA
[5] Observ Astron Marseille Provence, Marseille, France
[6] Lab Astrophys Marseille, Marseille, France
[7] Univ Nacl Autonoma Mexico, Inst Astron, Mexico City 04510, DF, Mexico
来源：
REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA | 2005年 / 41卷 / 02期
关键词：
ISM : Herbig-Haro objects; ISM; individual; (HH; 1; HH; 2); ISM : jets and outflows; ISM : kinematics and dynamics;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present new Ha Fabry-Perot observations of the HH 1/2 system. Line profiles, barycenter radial velocity maps and dispersion maps are derived from the channel maps of HH 1 and HH 2. The radial velocity barycenter maps of both HH 1 and HH 2 show a general trend of "red-shifted upstream/blue-shifted downstream" pattern. A "direct+scattered" component model for three emitting condensations is qualitatively successful at reproducing the general features of the barycenter and the velocity dispersion of HH 2.
引用
收藏
页码：371 / 382
页数：12
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