Publication:
A simple model for H-2 line profiles in bow shocks

dc.contributor.author Schultz, Angie en_US
dc.contributor.author Burton, Michael en_US
dc.contributor.author Brand, P. W. J. L. en_US
dc.date.accessioned 2021-11-25T12:55:33Z
dc.date.available 2021-11-25T12:55:33Z
dc.date.issued 2005 en_US
dc.description.abstract We present a model for empirically reproducing line profiles of molecular hydrogen emission in bow shocks. The model takes into account bow velocity, dissociation limit, a cooling function, viewing angle, bow shape and a limited form of extinction. Our results show that both geometrical factors and shock physics can significantly affect the profile morphology. In a companion paper we will apply this model to Fabry-Perot observations of bow shocks in the Orion BN-KL outflow. en_US
dc.identifier.issn 0035-8711 en_US
dc.identifier.uri http://hdl.handle.net/1959.4/38569
dc.language English
dc.language.iso EN en_US
dc.rights CC BY-NC-ND 3.0 en_US
dc.rights.uri https://creativecommons.org/licenses/by-nc-nd/3.0/au/ en_US
dc.source Legacy MARC en_US
dc.subject.other line : profiles en_US
dc.subject.other shock waves en_US
dc.subject.other stars : formation en_US
dc.subject.other ISM : jets and outflows en_US
dc.subject.other ISM : molecules en_US
dc.title A simple model for H-2 line profiles in bow shocks en_US
dc.type Journal Article en
dcterms.accessRights open access
dspace.entity.type Publication en_US
unsw.accessRights.uri https://purl.org/coar/access_right/c_abf2
unsw.description.notePublic The definitive version is available at www.blackwell-synergy.com en_US
unsw.identifier.doiPublisher http://dx.doi.org/10.1111/j.1365-2966.2005.08871.x en_US
unsw.relation.faculty Science
unsw.relation.ispartofissue 4 en_US
unsw.relation.ispartofjournal Monthly Notices of the Royal Astronomical Society en_US
unsw.relation.ispartofpagefrompageto 1195-1214 en_US
unsw.relation.ispartofvolume 358 en_US
unsw.relation.originalPublicationAffiliation Schultz, Angie, Physics, Faculty of Science, UNSW en_US
unsw.relation.originalPublicationAffiliation Burton, Michael, Physics, Faculty of Science, UNSW en_US
unsw.relation.originalPublicationAffiliation Brand, P. W. J. L., Institute for Astronomy, University of Edinburgh en_US
unsw.relation.school School of Physics *
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