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dc.contributor.authorDE PAOLIS, F.,
dc.contributor.authorGURZADYAN, V. G.,
dc.contributor.authorNUCITA, A. A.,
hal.structure.identifierM2A 2016
dc.contributor.authorCHEMIN, L.
dc.contributor.authorQADIR, A.,
dc.contributor.authorKASHIN, A. L.,
dc.contributor.authorKHACHATRYAN, H. G.,
hal.structure.identifierInstitut de Recherche en Communications et en Cybernétique de Nantes [IRCCyN]
dc.contributor.authorSARGSYAN, S.,
dc.contributor.authorYEGORIAN, G.,
hal.structure.identifierIstituto Nazionale di Oceanografia e di Geofisica Sperimentale [OGS]
dc.contributor.authorINGROSSO, G.,
hal.structure.identifierPhysik-Institut [Zürich]
dc.contributor.authorJETZER, Ph.,
dc.contributor.authorVETRUGNO, D.,
dc.date.issued2016
dc.identifier.issn0004-6361
dc.description.abstractEnWe used Planck data to study the M33 galaxy and find a substantial temperature asymmetry with respect to its minor axis projected onto the sky plane. This temperature asymmetry correlates well with the HI velocity field at 21 cm, at least within a galactocentric distance of 0.5 degree, and it is found to extend up to about 3 degrees from the galaxy center. We conclude that the revealed effect, that is, the temperature asymmetry and its extension, implies that we detected the differential rotation of the M33 galaxy and of its extended baryonic halo.
dc.language.isoen
dc.publisherEDP Sciences
dc.subject.enAstrophysics - Astrophysics of Galaxies
dc.title.enTriangulum galaxy viewed by Planck
dc.typeArticle de revue
dc.identifier.doi10.1051/0004-6361/201628780
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.identifier.arxiv1607.08099
bordeaux.journalAstronomy and Astrophysics - A&A
bordeaux.pageA57
bordeaux.volume593
bordeaux.peerReviewedoui
hal.identifierhal-01358310
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01358310v1
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