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most citedA Detailed Analysis of the Dust Formation Zone of IRC+10216 Derived from Mid-IR Bands of C2H2 and HCN

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astro-ph2005

H_2 Pure Rotational Lines in the Orion Bar

K. N. Allers, D. T. Jaffe, J. H. Lacy +2

Using the Texas Echelon Cross Echelle Spectrograph (TEXES) we mapped emission in the H_2 v = 0-0 S(1) and S(2) lines toward the Orion Bar PDR at 2" resolution. We also observed H_2…