3D maps of the local ISM from inversion of individual color excess measurements

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dc.contributor.authorLallement, Rosine
dc.contributor.authorVergely, Jean-Luc
dc.contributor.authorValette, B
dc.contributor.authorPuspitarini, Lucky
dc.contributor.authorEyer, L
dc.contributor.authorCasagrande, Luca
dc.date.accessioned2015-12-13T22:53:25Z
dc.date.issued2014
dc.date.updated2015-12-11T10:56:22Z
dc.description.abstractAims. Three-dimensional (3D) maps of the Galactic interstellar matter (ISM) are a potential tool of wide use, but accurate and detailed maps are still lacking. One of the ways to construct the maps is to invert individual distance-limited ISM measurements
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/81804
dc.publisherSpringer
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstronomy and Astrophysics
dc.title3D maps of the local ISM from inversion of individual color excess measurements
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.contributor.affiliationLallement, Rosine, GEPI Observatoire de Paris, CNRS, Université Paris Diderot
local.contributor.affiliationVergely, Jean-Luc, ACRI-ST
local.contributor.affiliationValette, B, Institut des Sciences de la Terre, IRD, Universite de Savoie
local.contributor.affiliationPuspitarini, Lucky, GEPI Observatoire de Paris, CNRS, Université Paris Diderot
local.contributor.affiliationEyer, L, Université de Genève
local.contributor.affiliationCasagrande, Luca, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidCasagrande, Luca, u5209059
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB10119
local.identifier.citationvolume561
local.identifier.doi10.1051/0004-6361/201322032
local.identifier.scopusID2-s2.0-84892146371
local.identifier.thomsonID000330584000091
local.type.statusPublished Version

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