Abstract
The bipolar nebula Ml-92 (Herbig, 1975) consists of a bright and a faint reflection lobe illuminated by a central stellar light source which is embedded in a dense equatorial dust disk. Ml-92 is considered to be a proto-planetary nebula (Eiroa and Hodapp, 1989).
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Eiroa, C., Hodapp, K.-W: 1989, Astron. Astrophys. 223, 271
Hartigan, J., Hartmann, L.: 1987, Astrophys. J. 316, 323
Herbig, G.H.: 1975, Astrophys. J. 200, 1
Morris, M.: 1987, P.A.S.P. 99, 1115
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© 1993 Springer Science+Business Media Dordrecht
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Solf, J. (1993). Spatially Resolved Spectroscopy of “Minkowskfs Footprint” (M1-92): Evidence for Bow Shocks in the Bipolar Outflow. In: Errico, L., Vittone, A.A. (eds) Stellar Jets and Bipolar Outflows. Astrophysics and Space Science Library, vol 186. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1924-5_46
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DOI: https://doi.org/10.1007/978-94-011-1924-5_46
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