A numerical model for the Serpens radio jet

Details A numerical model for the Serpens radio jet A numerical model for the Serpens radio jet

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...364..763r&link_type=abstract

Astronomy and Astrophysics, v.364, p.763-768 (2000)

Astronomy and Astrophysics

Astrophysics

13

Hydrodynamics, Molecular Processes, Radiative Transfer, Ism: Clouds, Ism: Herbig-Haro Objects, Ism: Jets And Outflows

Scientific paper

The Serpens (``triple source'') radio continuum jet shows a series of aligned knots with ~ 1-2'' angular separations, forming a curved structure circumscribed within a cone of ~ 10o full opening angle. We present a high resolution, 3D numerical simulation of a jet with variable ejection direction and velocity with parameters appropriate for the Serpens jet, from which we obtain predictions of 3.6 cm radio continuum maps. We find that the general morphology of the radio emission, and the time evolution of the successive knots, qualitatively agree with 3.6 cm VLA observations of the Serpens radio jet. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, the Netherlands and the United Kingdom) and with the participation of ISAS and NASA. Members of the Consortium on the ISOPHOT Serendipity Survey (CISS) are MPIA Heidelberg, ESA ISO SOC Villafranca, AIP Potsdam, IPAC Pasadena, Imperial College London.

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