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IC 3418: Star formation in a turbulent wake

dc.contributor.authorHester, Janice A.
dc.contributor.authorSeibert, Mark
dc.contributor.authorNeill, James D.
dc.contributor.authorWyder, Ted K.
dc.contributor.authorGil De Paz, Armando
dc.contributor.authorMadore, Barry F.
dc.contributor.authorMartin, D. Christopher
dc.contributor.authorSchiminovich, David
dc.contributor.authorRich, R. Michael
dc.date.accessioned2023-06-20T04:04:48Z
dc.date.available2023-06-20T04:04:48Z
dc.date.issued2010-06-10
dc.description© 2010. The American Astronomical Society. All rights reserved. This research has made use of the GOLD Mine Database of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. The authors thank L. Cortese for helpful comments.
dc.description.abstractGalaxy Evolution Explorer observations of IC 3418, a low surface brightness galaxy in the Virgo Cluster, revealed a striking 17 kpc UV tail of bright knots and diffuse emission. Hα imaging confirms that star formation is ongoing in the tail. IC 3418 was likely recently ram pressure stripped on its first pass through Virgo. We suggest that star formation is occurring in molecular clouds that formed in IC 3418's turbulent stripped wake. Tides and ram pressure stripping (RPS) of molecular clouds are both disfavored as tail formation mechanisms. The tail is similar to the few other observed star-forming tails, all of which likely formed during RPS. The tails' morphologies reflect the forces present during their formation and can be used to test for dynamical coupling between molecular and diffuse gas, thereby probing the origin of the star-forming molecular gas.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipNational Aeronautics and Space Administration (NASA)
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/35511
dc.identifier.doi10.1088/2041-8205/716/1/L14
dc.identifier.issn2041-8205
dc.identifier.officialurlhttp://dx.doi.org/10.1088/2041-8205/716/1/L14
dc.identifier.relatedurlhttp://iopscience.iop.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/44887
dc.issue.number1
dc.journal.titleAstrophysical journal letters
dc.language.isoeng
dc.page.finalL18
dc.page.initialL14
dc.publisherIOP Publishing
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordVirgo cluster
dc.subject.keywordRam-pressure
dc.subject.keywordSurface photometry
dc.subject.keywordSpiral galaxies
dc.subject.keywordFormation law
dc.subject.keywordH-alpha
dc.subject.keywordFormation rates
dc.subject.keywordLocal universe
dc.subject.keywordGalactic disks
dc.subject.keywordGas
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.titleIC 3418: Star formation in a turbulent wake
dc.typejournal article
dc.volume.number716
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