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OBSERVATIONS AND SHOCK-MODELS OF THE JET AND HERBIG-HARO OBJECTS HH-46/47
被引:84
作者:
HARTIGAN, P
RAYMOND, J
MEABURN, J
机构:
[1] UNIV MANCHESTER,DEPT ASTRON,MANCHESTER M13 9PL,LANCS,ENGLAND
[2] HARVARD SMITHSONIAN CTR ASTROPHYS,CAMBRIDGE,MA 02138
关键词:
Nebulae: internal motions;
Shock waves;
Stars: pre-main-sequence;
D O I:
10.1086/169301
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We present new monochromatic images, long-slit echelle spectra, and theoretical position-velocity diagrams of the Herbig-Haro objects HH 46 and HH 47. The outer bow shock HH 47D extends almost all the way back to the infrared source driving the outflow in a narrow-band [O II] image of the region, but is not easily visible in Hα and [S II]. We confirm the discovery of a counterjet in [S II] reported by Reipurth. Long-slit spectra of HH 47D show a "hook" shape in position-velocity space which can be understood in terms of a spatially resolved bow shock moving at an angle roughly 45° to the line of sight. The object HH 47A at the end of the jet also appears to be a bow shock rather than a Mach disk as has been suggested previously. The presence of two bow shocks within a single outflow is not predicted from a simple continuous jet model, but can be understood if the outflow is episodic or if both a disk wind and a stellar wind are present in the system.
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页码:624 / &
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