Optical and Near Infrared Study of the Cepheus E outflow, a very low excitation object

Details Optical and Near Infrared Study of the Cepheus E outflow, a very low excitation object Optical and Near Infrared Study of the Cepheus E outflow, a very low excitation object

2000-04-20

arxiv.org/abs/astro-ph/0004298v1

Astronomy and Astrophysics

Astrophysics

Accepted Astron. J., 8 files: paper, tables plus 6 figures

Scientific paper

10.1086/301500

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 r\^ole 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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