Jet/cloud collision, 3D gasdynamic simulations of HH 110

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Show simple item record Raga, AC Dal Pino, EMD Noriega-Crespo, A Mininni, PD Velazquez, PF 2011-01-22T10:26:50Z 2011-01-22T10:26:50Z 2002
dc.identifier.issn 0004-6361
dc.description.abstract We present 3D, gasdynamic simulations of jet/cloud collisions, with the purpose of modelling the HH 270/110 system. From the models, we obtain predictions of Halpha and H-2 1-0 s(1) emission line maps, which qualitatively reproduce some of the main features of the corresponding observations of HH 110. We find that the model that better reproduces the observed structures corresponds to a jet that was deflected at the surface of the cloud similar to 1000 yr ago, but is now boring a tunnel directly into the cloud. This model removes the apparent contradiction between the jet/cloud collision model and the lack of detection of molecular emission in the crossing region of the HH 270 and HH 110 axes. en_US
dc.language.iso en en_US
dc.title Jet/cloud collision, 3D gasdynamic simulations of HH 110 en_US
dc.type Article en_US
dc.identifier.idprometeo 2114
dc.identifier.doi 10.1051/0004-6361:20020851
dc.source.novolpages 392(1):267-276
dc.subject.wos Astronomy & Astrophysics
dc.description.index WoS: SCI, SSCI o AHCI
dc.subject.keywords ISM : Herbig-Haro objects
dc.subject.keywords ISM : jets and outflows
dc.subject.keywords ISM : kinematics and dynamics
dc.subject.keywords ISM : individual (HH 110)
dc.subject.keywords shock waves
dc.relation.journal Astronomy & Astrophysics

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