arXiv · astro-ph/0004298
Optical and Near Infrared Study of the Cepheus E outflow, a very low excitation object
Abstract
We present images and spectra of the Cepheus E (Cep E) region at both optical and infrared wavelengths. Only the brightest region of the southern lobe of the Cep E outflow reveals optical emission, suggesting that the extinction close to the outflow source plays an important rôle in the observed difference between the optical and IR morphologies. Cep E is a unique object since it provides a link between the spectroscopic properties of the optical Herbig-Haro (HH) objects and those of deeply embedded outflows.
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S. Ayala, A. Noriega-Crespo, P. M. Garnavich, S. Curiel, A. C. Raga, K. H. Bohm, J. Raymond. 2000-04-20. Optical and Near Infrared Study of the Cepheus E outflow, a very low excitation object. https://doi.org/10.1086/301500
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