INFRARED-SPECTROSCOPY OF HERBIG-HARO OBJECTS

被引:16
作者
SCHWARTZ, RD
SCHULTZ, ASB
COHEN, M
WILLIAMS, PM
机构
[1] WASHINGTON UNIV, DEPT PHYS, ST LOUIS, MO 63130 USA
[2] WASHINGTON UNIV, MCDONNELL CTR SPACE SCI, ST LOUIS, MO 63130 USA
[3] UNIV CALIF BERKELEY, RADIO ASTRON LAB, BERKELEY, CA 94720 USA
[4] ROYAL OBSERV, EDINBURGH EH9 3HJ, MIDLOTHIAN, SCOTLAND
关键词
INFRARED; STARS; SHOCK WAVES; PRE-MAIN-SEQUENCE;
D O I
10.1086/175790
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report near-infrared spectrophotometry of H-2 emission in a set of low-excitation Herbig-Haro objects for which optical emission line fluxes are available. In most objects, the H-2 line ratio 2-1 S(3)/1-0 S(1) is consistent with collisional excitation in low-velocity shocks, with no indication of a fluorescence component. The excitation plot for HH 43 shows definite curvature, with a nonlinear (logarithmic) best fit suggesting that the higher excitation lines are created in the hottest postshock gas. This curvature of the excitation plot is akin to that seen in HH 98A and the OMC, where it has been taken as evidence of nondissociative J-shocks. In general, the 1-0 S(1) flux appears to be comparable to the H alpha flux. The implications of this are discussed with respect to the nature of the shocks which produce the optical and H-2 emission.
引用
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页码:318 / 330
页数:13
相关论文
共 42 条
[1]  
Bohm K.-H., Soif J., ApJ, 294, (1985)
[2]  
Brand P.W.J.L., Moorhouse A., Burton M.G., Geballe T.R., Bird M., Wade R., ApJ, 334, (1988)
[3]  
Chang C.A., Martin P.G., ApJ, 378, (1991)
[4]  
Cohen M., MNRAS, 164, (1973)
[5]  
Cohen M., Hollenbach D.J., Haas M.R., Erickson E.F., ApJ, 329, (1988)
[6]  
Cohen M., Jones B.F., Hereld M., ApJ, 371, (1991)
[7]  
Cohen M., Schwartz R.D., ApJ, 265, (1983)
[8]  
Cohen M., Walker R.G., Barlow M.J., Deacon J.R., AJ, 104, (1992)
[9]  
Curiel S., (1992)
[10]  
Davis C.J., Eisloffel J., Ray T.P., ApJ, 426, (1994)