Evidence for Disks around Young Massive Stars from 3D Radiative Transfer Image Modeling
| hal.structure.identifier | Max-Planck-Institut für Astronomie [MPIA] | |
| dc.contributor.author | STEINACKER, J. | |
| dc.contributor.author | CHINI, R. | |
| dc.contributor.author | NIELBOCK, M. | |
| dc.contributor.author | NÜRNBERGER, D. E. A. | |
| dc.contributor.author | HOFFMEISTER, V. | |
| hal.structure.identifier | Observatoire aquitain des sciences de l'univers [OASU] | |
| hal.structure.identifier | Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB] | |
| hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
| hal.structure.identifier | Université Sciences et Technologies - Bordeaux 1 [UB] | |
| dc.contributor.author | HURÉ, J.-M. | |
| hal.structure.identifier | A.N. Severtsov Institute of Ecology and Evolution | |
| hal.structure.identifier | Max-Planck-Institut für Astronomie [MPIA] | |
| dc.contributor.author | SEMENOV, D. | |
| dc.contributor.author | SCHEYDA, C. M. | |
| dc.contributor.author | SIEBENMORGEN, R. | |
| dc.date.issued | 2008 | |
| dc.date.conference | 2007-09-14 | |
| dc.description.abstractEn | While a paradigm for the formation of low-mass stars has been established that is based on accretion of gas and dust through a circumstellar disk, there is no agreed formation scenario for stars with masses greater than 10 solar masses. New evidence for the existence of large-scale flattened structures around young massive stars and compact H II regions is presented and analyzed by radiative transfer models: i) An analysis of the most-extended circumstellar disk known so far including a stability analysis of extended disk structures. ii) A comparison of K-band images of the first hypercompact H II region with a disk candidate and scattered light models. iii) A modeling of the first candidate for a remnant disk around a massive star. | |
| dc.language.iso | en | |
| dc.title.en | Evidence for Disks around Young Massive Stars from 3D Radiative Transfer Image Modeling | |
| dc.type | Communication dans un congrès | |
| dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO] | |
| dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph] | |
| bordeaux.page | 270 | |
| bordeaux.volume | 387 | |
| bordeaux.country | DE | |
| bordeaux.conference.city | Heidelberg | |
| bordeaux.peerReviewed | oui | |
| hal.identifier | hal-00286488 | |
| hal.version | 1 | |
| hal.invited | non | |
| hal.proceedings | oui | |
| hal.popular | non | |
| hal.audience | Internationale | |
| hal.origin.link | https://hal.archives-ouvertes.fr//hal-00286488v1 | |
| bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2008&rft.volume=387&rft.spage=270&rft.epage=270&rft.au=STEINACKER,%20J.&CHINI,%20R.&NIELBOCK,%20M.&N%C3%9CRNBERGER,%20D.%20E.%20A.&HOFFMEISTER,%20V.&rft.genre=unknown |
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