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Title:
X-ray Emission Mechanisms in Herbig - Haro objects .
Authors:
Bonito, R.; Orlando, S.; Peres, G.; Favata, F.; Rosner, R.
Affiliation:
AA( Dip. S.F.A., Sez. Astronomia, Universitàdi Palermo, P.zza del Parlamento 1, 90134 Palermo, Italy ; INAF - Osservatorio Astronomico di Palermo, Italy), AB(INAF - Osservatorio Astronomico di Palermo, Italy), AC( Dip. S.F.A., Sez. Astronomia, Universitàdi Palermo, P.zza del Parlamento 1, 90134 Palermo, Italy ), AD(Astrophysics Division - Research and Science Support Department of ESA, ESTEC, Postbus 299, 2200 AG Noordwijk, The Netherlands), AE(Dept. of Astronomy and Astrophysics, Univ. of Chicago, Chicago, IL 60637, USA; Center for Astrophysical Thermonuclear Flashes, University of Chicago, 5640 S. Ellis Avenue, Chicago, IL 60637, USA)
Publication:
Memorie della Societa Astronomica Italiana Supplement, v.9, p.226 (2006)
Publication Date:
00/2006
Origin:
MmSAI
Keywords:
ISM: Herbig-Haro objects, ISM: individual objects: HH 154, ISM: jets and outflows, X-rays: ISM
Abstract Copyright:
(c) 2006: SAIt
Bibliographic Code:
2006MSAIS...9..226B

Abstract

X-ray emission in Herbig - Haro objects is a quite recent and uncommon finding still waiting full explanation. With the scope of explaining this X-ray emission, our project is devoted to model the interaction between a supersonic jet originating from a young stellar object and the ambient medium. We have performed a wide exploration of the parameter space to infer the configuration(s) which can give rise to X-ray emission very similar to what recently observed.

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