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dc.contributor.authorDale, J. E.
dc.contributor.authorErcolano, B.
dc.contributor.authorBonnell, I. A.
dc.date.accessioned2014-05-12T15:01:03Z
dc.date.available2014-05-12T15:01:03Z
dc.date.issued2012-12-21
dc.identifier.citationDale , J E , Ercolano , B & Bonnell , I A 2012 , ' Ionization-induced star formation - IV. Triggering in bound clusters ' Monthly Notices of the Royal Astronomical Society , vol. 427 , no. 4 , pp. 2852-2865 . https://doi.org/10.1111/j.1365-2966.2012.22104.xen
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 117862052
dc.identifier.otherPURE UUID: ef7e407f-0514-410c-9839-47796804aed7
dc.identifier.otherWOS: 000312093200013
dc.identifier.otherScopus: 84885724813
dc.identifier.urihttp://hdl.handle.net/10023/4767
dc.description.abstractWe present a detailed study of star formation occurring in bound star-forming clouds under the influence of internal ionizing feedback from massive stars across a spectrum of cloud properties. We infer which objects are triggered by comparing our feedback simulations with control simulations in which no feedback was present. We find that feedback always results in a lower star formation efficiency and usually but not always results in a larger number of stars or clusters. Cluster mass functions are not strongly affected by feedback, but stellar mass functions are biased towards lower masses. Ionization also affects the geometrical distribution of stars in ways that are robust against projection effects, but may make the stellar associations more or less subclustered depending on the background cloud environment. We observe a prominent pillar in one simulation which is the remains of an accretion flow feeding the central ionizing cluster of its host cloud and suggest that this may be a general formation mechanism for pillars such as those observed in M16. We find that the association of stars with structures in the gas such as shells or pillars is a good but by no means foolproof indication that those stars have been triggered and we conclude overall that it is very difficult to deduce which objects have been induced to form and which formed spontaneously simply from observing the system at a single time.
dc.format.extent14
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2012 The Authors. Monthly Notices of the Royal Astronomical Society © 2012 RAS.en
dc.subjectStars: formationen
dc.subjectRadiation-driven implosionen
dc.subjectMolecular cloud coresen
dc.subjectInitial mass functionen
dc.subjectGalactic hii-regionsen
dc.subjectSequential formationen
dc.subjectOB associationsen
dc.subjectMilky-wayen
dc.subjectBordersen
dc.subjectPeripheryen
dc.subjectCollapseen
dc.subjectQB Astronomyen
dc.subject.lccQBen
dc.titleIonization-induced star formation - IV. Triggering in bound clustersen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1111/j.1365-2966.2012.22104.x
dc.description.statusPeer revieweden


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