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dc.contributor.authorHaworth, T.~J.
dc.contributor.authorShima, K.
dc.contributor.authorTasker, E.~J.
dc.contributor.authorFukui, Y.
dc.contributor.authorTorii, K.
dc.contributor.authorTakahira, K.
dc.contributor.authorHabe, A.
dc.contributor.authorDale, James
dc.date.accessioned2017-07-10T12:11:44Z
dc.date.available2017-07-10T12:11:44Z
dc.date.issued2015-12-01
dc.identifier.citationHaworth , T J , Shima , K , Tasker , E J , Fukui , Y , Torii , K , Takahira , K , Habe , A & Dale , J 2015 , ' Isolating signatures of major cloud-cloud collisions - II. The lifetimes of broad bridge features ' Monthly Notices of the Royal Astronomical Society , vol. 454 , no. 2 , pp. 1634-1643 . https://doi.org/10.1093/mnras/stv2068
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 11150663
dc.identifier.otherPURE UUID: fa4486fe-f6cd-45f3-b800-c2309d89cf8c
dc.identifier.otherBibtex: urn:87e1155c0d2c0efe27c1374bae7784ed
dc.identifier.otherScopus: 84960846384
dc.identifier.urihttp://hdl.handle.net/2299/18850
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
dc.description.abstractWe investigate the longevity of broad bridge features in position–velocity diagrams that appear as a result of cloud–cloud collisions. Broad bridges will have a finite lifetime due to the action of feedback, conversion of gas into stars and the time-scale of the collision. We make a series of analytic arguments with which to estimate these lifetimes. Our simple analytic arguments suggest that for collisions between clouds larger than R ∼ 10 pc the lifetime of the broad bridge is more likely to be determined by the lifetime of the collision rather than the radiative or wind feedback disruption time-scale. However, for smaller clouds feedback becomes much more effective. This is because the radiative feedback time-scale scales with the ionizing flux Nly as R7/4N−1/4ly R7/4Nly−1/4 so a reduction in cloud size requires a relatively large decrease in ionizing photons to maintain a given time-scale. We find that our analytic arguments are consistent with new synthetic observations of numerical simulations of cloud–cloud collisions (including star formation and radiative feedback). We also argue that if the number of observable broad bridges remains ∼ constant, then the disruption time-scale must be roughly equivalent to the collision rate. If this is the case, our analytic arguments also provide collision rate estimates, which we find are readily consistent with previous theoretical models at the scales they consider (clouds larger than about 10 pc) but are much higher for smaller clouds.en
dc.format.extent10
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.subjectstars: formation, ISM: bubbles, ISM: clouds, ISM: kinematics and dynamics, galaxies: ISM
dc.titleIsolating signatures of major cloud-cloud collisions - II. The lifetimes of broad bridge featuresen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.identifier.urlhttps://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stv2068
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Published version
dcterms.dateAccepted2015-09-03
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stv2068
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeopenAccess


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