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First AMBER/VLTI Observations of Hot Massive Stars

dc.contributor.authorPetrov, RG
dc.contributor.authorMillour, F
dc.contributor.authorChesneau, O
dc.contributor.authorWeigelt, G
dc.contributor.authorBonneau, D
dc.contributor.authorStee, P
dc.contributor.authorKraus, S
dc.contributor.authorMourard, D
dc.contributor.authorMeilland, A
dc.contributor.authorVannier, M
dc.contributor.authorMalbet, F
dc.contributor.authorLisi, F
dc.contributor.authorAntonelli, P
dc.contributor.authorKern, P
dc.contributor.authorBeckmann, U
dc.contributor.authorLagarde, S
dc.contributor.authorPerraut, K
dc.contributor.authorGennari, S
dc.contributor.authorCoarer, EL
dc.contributor.authorDriebe, T
dc.contributor.authorAccardo, M
dc.contributor.authorRobbe-Dubois, S
dc.contributor.authorOhnaka, K
dc.contributor.authorBusoni, S
dc.contributor.authorRoussel, A
dc.contributor.authorZins, G
dc.contributor.authorBehrend, J
dc.contributor.authorFerruzi, D
dc.contributor.authorBresson, Y
dc.contributor.authorDuvert, G
dc.contributor.authorNussbaum, E
dc.contributor.authorMarconi, A
dc.contributor.authorFeautrier, P
dc.contributor.authorDugué, M
dc.contributor.authorChelli, A
dc.contributor.authorTatulli, E
dc.contributor.authorHeininger, M
dc.contributor.authorDelboulbe, A
dc.contributor.authorBonhomme, S
dc.contributor.authorSchertl, D
dc.contributor.authorTesti, L
dc.contributor.authorMathias, P
dc.contributor.authorMonin, J-L
dc.contributor.authorGluck, L
dc.contributor.authorHofmann, KH
dc.contributor.authorSalinari, P
dc.contributor.authorPuget, P
dc.contributor.authorClausse, JM
dc.contributor.authorFraix-Burnet, D
dc.contributor.authorFoy, R
dc.contributor.authorIsella, A
dc.date.accessioned2018-01-15T13:48:27Z
dc.date.issued2007-10-12
dc.description.abstractAMBER is the first near infrared focal instrument of the VLTI. It combines three telescopes and produces spectrally resolved interferometric measures. This paper discusses some preliminary results of the first scientific observations of AMBER with three Unit Telescopes at medium (1500) and high (12000) spectral resolution. We derive a first set of constraints on the structure of the circumstellar material around the Wolf Rayet γ2 Velorum and the LBV η Carinae.en_GB
dc.identifier.citationIn: Richichi A., Delplancke F., Paresce F., Chelli A. (eds) The Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation Instrumentation. Eso Astrophysics Symposia (European Southern Observatory), pp. 153 - 161en_GB
dc.identifier.doi10.1007/978-3-540-74256-2_17
dc.identifier.urihttp://hdl.handle.net/10871/31004
dc.language.isoenen_GB
dc.publisherSpringeren_GB
dc.rights© 2007 Springeren_GB
dc.titleFirst AMBER/VLTI Observations of Hot Massive Starsen_GB
dc.typeBook chapteren_GB
dc.contributor.editorRichichi, Aen_GB
dc.contributor.editorDelplancke, Fen_GB
dc.contributor.editorParesce, Fen_GB
dc.contributor.editorChelli, Aen_GB
dc.identifier.isbn978-3-540-74256-2
dc.descriptionThis is the author accepted manuscript. The final version is available from Springer via the DOI in this record.en_GB


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