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Morphology as a tracer of evolution in the early phases of galaxy assembly

Author: Bruno RibeiroOlivier Le Fèvre, astrophysicien).Philippe AmramAdriano FontanaR MaiolinoAll authors
Publisher: 2016.
Dissertation: Thèse de doctorat : Astrophysique et Cosmologie : Aix-Marseille : 2016.
Edition/Format:   Computer file : Document : Thesis/dissertation : English
Summary:
Les propriétés globales des galaxies montrent une forte évolution du taux de formation stellaire et de la densité de masse stellaire à l'époque de l'assemblage des galaxies précédent le pic de formation stellaire dans l'univers, produite par plusieurs processus physiques concurrents (fusion, accrétion, rétroaction, environnement, ...). Les propriétés morphologiques des galaxies ont aussi fortement
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Details

Genre/Form: Thèses et écrits académiques
Material Type: Document, Thesis/dissertation, Internet resource
Document Type: Internet Resource, Computer File
All Authors / Contributors: Bruno Ribeiro; Olivier Le Fèvre, astrophysicien).; Philippe Amram; Adriano Fontana; R Maiolino; Lidia Tasca; Emmanuel Bertin; Aix-Marseille Université.; Ecole Doctorale Physique et Sciences de la Matière (Marseille).; Laboratoire d'Astrophysique de Marseille (LAM).
OCLC Number: 993584435
Notes: Titre provenant de l'écran-titre.
Description: 1 online resource
Responsibility: Bruno Ribeiro ; sous la direction de Olivier Le Fèvre.

Abstract:

Les propriétés globales des galaxies montrent une forte évolution du taux de formation stellaire et de la densité de masse stellaire à l'époque de l'assemblage des galaxies précédent le pic de formation stellaire dans l'univers, produite par plusieurs processus physiques concurrents (fusion, accrétion, rétroaction, environnement, ...). Les propriétés morphologiques des galaxies ont aussi fortement évolué à la même époque. Dans cette thèse, j'étudie comment l'évolution des propriétés morphologique est reliée aux propriétés spectrophotométriques des galaxies depuis z ~ 6. Les données spectroscopiques obtenues au sein du VIMOS Ultra Deep Survey (VUDS), un nouveau sondage spectroscopique unique de ~ 10000 galaxies entre redshift z~2 et z~6 qui fournissent un excellent moyen de sonder l'évolution galactique à travers cette époque cosmique. A partir des mes résultats, je conclus que les différentes propriétés morphologiques de galaxies à formation stellaire aux redshifts 2<z<6 montrent qu'il existe plusieurs façons pour les galaxies de se former. La grande diversité de tailles, la fraction importante de super-amas d'étoiles et de gaz très lumineux indiquant des fusions et ceux moins lumineux résultant probablement d'instabilités dans la formation des disques galactiques, avec la prévalence de galaxies irrégulières couvrant un grand domaine de masse stellaire et formation stellaire, pointent ensemble un scénario ou l'assemblage des galaxies procéde de différents méchanismes physiques. La formation des galaxies apparait plus complexe qu'un scénario simple impliquant la formation d'un disque avec de l'accrétion de gaz pourrait le faire croire.

The global properties of galaxies show a strong evolution of the star formation rate and stellar mass density at the epoch of galaxy assembly, driven by several competing physical processes (merging, accretion, feedback, environment,...). The morphological properties of galaxies are also strongly evolving over the same timescales. I investigate how the evolution of the morphological properties is connected to the spectrophotometric properties of galaxies since z~6. The spectroscopic data obtained within the VIMOS Ultra Deep Survey (VUDS), a new unique spectroscopic survey of ~10000 galaxies between redshifts z~2 and z~6 conducted at the ESO-VLT, combined with the available Hubble Space Telescope imaging surveys such as COSMOS or CANDELS provide a great way of probing galactic evolution across this cosmic epoch.From the results that I have obtained, I conclude that the different morphological properties of star-forming galaxies at 2<z<6 show that there are several mechanisms that take part in galaxy formation. The great diversity in galaxy sizes, the high number of bright two clump systems as well as faint multi-clump systems indicating merger and disk instabilities processes, respectively, and the wide range in physical properties that are populated by irregular galaxies all point to a diverse history for galaxy formation. This suggests that forming galaxies is far more complex that the simple explanation of evolution from gas accretion alone.

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Primary Entity<\/h3>\n
<http:\/\/www.worldcat.org\/oclc\/993584435<\/a>> # Morphology as a tracer of evolution in the early phases of galaxy assembly<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:CreativeWork<\/a>, schema:MediaObject<\/a>, bgn:ComputerFile<\/a>, bgn:Thesis<\/a> ;\u00A0\u00A0\u00A0\nbgn:inSupportOf<\/a> \"Th\u00E8se de doctorat : Astrophysique et Cosmologie : Aix-Marseille : 2016.<\/span>\" ;\u00A0\u00A0\u00A0\nlibrary:oclcnum<\/a> \"993584435<\/span>\" ;\u00A0\u00A0\u00A0\nlibrary:placeOfPublication<\/a> <http:\/\/id.loc.gov\/vocabulary\/countries\/fr<\/a>> ;\u00A0\u00A0\u00A0\nschema:about<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Thing\/evolution<\/a>> ; # \u00C9volution<\/span>\n\u00A0\u00A0\u00A0\nschema:about<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Thing\/lyman_alpha<\/a>> ; # Lyman-Alpha<\/span>\n\u00A0\u00A0\u00A0\nschema:about<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Topic\/matiere_interstellaire<\/a>> ; # Mati\u00E8re interstellaire<\/span>\n\u00A0\u00A0\u00A0\nschema:about<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Topic\/spectrophotometrie<\/a>> ; # Spectrophotom\u00E9trie<\/span>\n\u00A0\u00A0\u00A0\nschema:about<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Thing\/morphologie<\/a>> ; # Morphologie<\/span>\n\u00A0\u00A0\u00A0\nschema:about<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Topic\/imagerie_infrarouge<\/a>> ; # Imagerie infrarouge<\/span>\n\u00A0\u00A0\u00A0\nschema:about<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Topic\/structure_a_grande_echelle_astronomie<\/a>> ; # Structure \u00E0 grande \u00E9chelle (astronomie)<\/span>\n\u00A0\u00A0\u00A0\nschema:about<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Thing\/galaxies<\/a>> ; # Galaxies<\/span>\n\u00A0\u00A0\u00A0\nschema:about<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Thing\/haut_redshift<\/a>> ; # Haut redshift<\/span>\n\u00A0\u00A0\u00A0\nschema:about<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Topic\/galaxies_formation<\/a>> ; # Galaxies--Formation<\/span>\n\u00A0\u00A0\u00A0\nschema:about<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Topic\/etoiles_formation<\/a>> ; # \u00C9toiles--Formation<\/span>\n\u00A0\u00A0\u00A0\nschema:author<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/ribeiro_bruno_1989<\/a>> ; # Bruno Ribeiro<\/span>\n\u00A0\u00A0\u00A0\nschema:contributor<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/fontana_adriano<\/a>> ; # Adriano Fontana<\/span>\n\u00A0\u00A0\u00A0\nschema:contributor<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/amram_philippe<\/a>> ; # Philippe Amram<\/span>\n\u00A0\u00A0\u00A0\nschema:contributor<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/maiolino_r<\/a>> ; # R Maiolino<\/span>\n\u00A0\u00A0\u00A0\nschema:contributor<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Organization\/aix_marseille_universite<\/a>> ; # Aix-Marseille Universit\u00E9.<\/span>\n\u00A0\u00A0\u00A0\nschema:contributor<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Organization\/laboratoire_d_astrophysique_de_marseille_lam<\/a>> ; # Laboratoire d\'Astrophysique de Marseille (LAM).<\/span>\n\u00A0\u00A0\u00A0\nschema:contributor<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Organization\/ecole_doctorale_physique_et_sciences_de_la_matiere_marseille<\/a>> ; # Ecole Doctorale Physique et Sciences de la Mati\u00E8re (Marseille).<\/span>\n\u00A0\u00A0\u00A0\nschema:contributor<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/le_fevre_olivier_1960_2020_astrophysicien<\/a>> ; # astrophysicien). Olivier Le F\u00E8vre<\/span>\n\u00A0\u00A0\u00A0\nschema:contributor<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/tasca_lidia<\/a>> ; # Lidia Tasca<\/span>\n\u00A0\u00A0\u00A0\nschema:contributor<\/a> <http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/bertin_emmanuel<\/a>> ; # Emmanuel Bertin<\/span>\n\u00A0\u00A0\u00A0\nschema:datePublished<\/a> \"2016<\/span>\" ;\u00A0\u00A0\u00A0\nschema:description<\/a> \"Les propri\u00E9t\u00E9s globales des galaxies montrent une forte \u00E9volution du taux de formation stellaire et de la densit\u00E9 de masse stellaire \u00E0 l\'\u00E9poque de l\'assemblage des galaxies pr\u00E9c\u00E9dent le pic de formation stellaire dans l\'univers, produite par plusieurs processus physiques concurrents (fusion, accr\u00E9tion, r\u00E9troaction, environnement, ...). Les propri\u00E9t\u00E9s morphologiques des galaxies ont aussi fortement \u00E9volu\u00E9 \u00E0 la m\u00EAme \u00E9poque. Dans cette th\u00E8se, j\'\u00E9tudie comment l\'\u00E9volution des propri\u00E9t\u00E9s morphologique est reli\u00E9e aux propri\u00E9t\u00E9s spectrophotom\u00E9triques des galaxies depuis z ~ 6. Les donn\u00E9es spectroscopiques obtenues au sein du VIMOS Ultra Deep Survey (VUDS), un nouveau sondage spectroscopique unique de ~ 10000 galaxies entre redshift z~2 et z~6 qui fournissent un excellent moyen de sonder l\'\u00E9volution galactique \u00E0 travers cette \u00E9poque cosmique. A partir des mes r\u00E9sultats, je conclus que les diff\u00E9rentes propri\u00E9t\u00E9s morphologiques de galaxies \u00E0 formation stellaire aux redshifts 2\" ;\u00A0\u00A0\u00A0\nschema:description<\/a> \"The global properties of galaxies show a strong evolution of the star formation rate and stellar mass density at the epoch of galaxy assembly, driven by several competing physical processes (merging, accretion, feedback, environment,...). The morphological properties of galaxies are also strongly evolving over the same timescales. I investigate how the evolution of the morphological properties is connected to the spectrophotometric properties of galaxies since z~6. The spectroscopic data obtained within the VIMOS Ultra Deep Survey (VUDS), a new unique spectroscopic survey of ~10000 galaxies between redshifts z~2 and z~6 conducted at the ESO-VLT, combined with the available Hubble Space Telescope imaging surveys such as COSMOS or CANDELS provide a great way of probing galactic evolution across this cosmic epoch.From the results that I have obtained, I conclude that the different morphological properties of star-forming galaxies at 2\" ;\u00A0\u00A0\u00A0\nschema:exampleOfWork<\/a> <http:\/\/worldcat.org\/entity\/work\/id\/4415328799<\/a>> ;\u00A0\u00A0\u00A0\nschema:genre<\/a> \"Th\u00E8ses et \u00E9crits acad\u00E9miques<\/span>\" ;\u00A0\u00A0\u00A0\nschema:inLanguage<\/a> \"en<\/span>\" ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Morphology as a tracer of evolution in the early phases of galaxy assembly<\/span>\" ;\u00A0\u00A0\u00A0\nschema:productID<\/a> \"993584435<\/span>\" ;\u00A0\u00A0\u00A0\nschema:url<\/a> <http:\/\/www.theses.fr\/2016AIXM4744\/document<\/a>> ;\u00A0\u00A0\u00A0\nschema:url<\/a> <http:\/\/www.theses.fr\/2016AIXM4744\/abes<\/a>> ;\u00A0\u00A0\u00A0\nwdrs:describedby<\/a> <http:\/\/www.worldcat.org\/title\/-\/oclc\/993584435<\/a>> ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n\n

Related Entities<\/h3>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Organization\/aix_marseille_universite<\/a>> # Aix-Marseille Universit\u00E9.<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Organization<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Aix-Marseille Universit\u00E9.<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Organization\/ecole_doctorale_physique_et_sciences_de_la_matiere_marseille<\/a>> # Ecole Doctorale Physique et Sciences de la Mati\u00E8re (Marseille).<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Organization<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Ecole Doctorale Physique et Sciences de la Mati\u00E8re (Marseille).<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Organization\/laboratoire_d_astrophysique_de_marseille_lam<\/a>> # Laboratoire d\'Astrophysique de Marseille (LAM).<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Organization<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Laboratoire d\'Astrophysique de Marseille (LAM).<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/amram_philippe<\/a>> # Philippe Amram<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Person<\/a> ;\u00A0\u00A0\u00A0\nschema:familyName<\/a> \"Amram<\/span>\" ;\u00A0\u00A0\u00A0\nschema:givenName<\/a> \"Philippe<\/span>\" ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Philippe Amram<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/bertin_emmanuel<\/a>> # Emmanuel Bertin<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Person<\/a> ;\u00A0\u00A0\u00A0\nschema:familyName<\/a> \"Bertin<\/span>\" ;\u00A0\u00A0\u00A0\nschema:givenName<\/a> \"Emmanuel<\/span>\" ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Emmanuel Bertin<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/fontana_adriano<\/a>> # Adriano Fontana<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Person<\/a> ;\u00A0\u00A0\u00A0\nschema:familyName<\/a> \"Fontana<\/span>\" ;\u00A0\u00A0\u00A0\nschema:givenName<\/a> \"Adriano<\/span>\" ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Adriano Fontana<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/le_fevre_olivier_1960_2020_astrophysicien<\/a>> # astrophysicien). Olivier Le F\u00E8vre<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Person<\/a> ;\u00A0\u00A0\u00A0\nschema:birthDate<\/a> \"1960<\/span>\" ;\u00A0\u00A0\u00A0\nschema:deathDate<\/a> \"2020;<\/span>\" ;\u00A0\u00A0\u00A0\nschema:familyName<\/a> \"Le F\u00E8vre<\/span>\" ;\u00A0\u00A0\u00A0\nschema:givenName<\/a> \"Olivier<\/span>\" ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"astrophysicien). Olivier Le F\u00E8vre<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/maiolino_r<\/a>> # R Maiolino<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Person<\/a> ;\u00A0\u00A0\u00A0\nschema:familyName<\/a> \"Maiolino<\/span>\" ;\u00A0\u00A0\u00A0\nschema:givenName<\/a> \"R.<\/span>\" ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"R Maiolino<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/ribeiro_bruno_1989<\/a>> # Bruno Ribeiro<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Person<\/a> ;\u00A0\u00A0\u00A0\nschema:birthDate<\/a> \"1989<\/span>\" ;\u00A0\u00A0\u00A0\nschema:deathDate<\/a> \"\" ;\u00A0\u00A0\u00A0\nschema:familyName<\/a> \"Ribeiro<\/span>\" ;\u00A0\u00A0\u00A0\nschema:givenName<\/a> \"Bruno<\/span>\" ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Bruno Ribeiro<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Person\/tasca_lidia<\/a>> # Lidia Tasca<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Person<\/a> ;\u00A0\u00A0\u00A0\nschema:familyName<\/a> \"Tasca<\/span>\" ;\u00A0\u00A0\u00A0\nschema:givenName<\/a> \"Lidia<\/span>\" ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Lidia Tasca<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Thing\/evolution<\/a>> # \u00C9volution<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Thing<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"\u00C9volution<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Thing\/galaxies<\/a>> # Galaxies<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Thing<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Galaxies<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Thing\/haut_redshift<\/a>> # Haut redshift<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Thing<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Haut redshift<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Thing\/lyman_alpha<\/a>> # Lyman-Alpha<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Thing<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Lyman-Alpha<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Thing\/morphologie<\/a>> # Morphologie<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Thing<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Morphologie<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Topic\/etoiles_formation<\/a>> # \u00C9toiles--Formation<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Intangible<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"\u00C9toiles--Formation<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Topic\/galaxies_formation<\/a>> # Galaxies--Formation<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Intangible<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Galaxies--Formation<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Topic\/imagerie_infrarouge<\/a>> # Imagerie infrarouge<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Intangible<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Imagerie infrarouge<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Topic\/matiere_interstellaire<\/a>> # Mati\u00E8re interstellaire<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Intangible<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Mati\u00E8re interstellaire<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Topic\/spectrophotometrie<\/a>> # Spectrophotom\u00E9trie<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Intangible<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Spectrophotom\u00E9trie<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/experiment.worldcat.org\/entity\/work\/data\/4415328799#Topic\/structure_a_grande_echelle_astronomie<\/a>> # Structure \u00E0 grande \u00E9chelle (astronomie)<\/span>\n\u00A0\u00A0\u00A0\u00A0a \nschema:Intangible<\/a> ;\u00A0\u00A0\u00A0\nschema:name<\/a> \"Structure \u00E0 grande \u00E9chelle (astronomie)<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/id.loc.gov\/vocabulary\/countries\/fr<\/a>>\u00A0\u00A0\u00A0\u00A0a \nschema:Place<\/a> ;\u00A0\u00A0\u00A0\ndcterms:identifier<\/a> \"fr<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n
<http:\/\/www.theses.fr\/2016AIXM4744\/document<\/a>>\u00A0\u00A0\u00A0\nrdfs:comment<\/a> \"Acc\u00E8s au texte int\u00E9gral<\/span>\" ;\u00A0\u00A0\u00A0\u00A0.\n\n\n<\/div>\n