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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



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ID: 559176.0, MPI für Astronomie / Publikationen_mpia
Spatially and spectrally resolved hydrogen gas within 0.1 AU of T Tauri and Herbig Ae/Be stars
Authors:Eisner, J. A.; Monnier, J. D.; Woillez, J.; Akeson, R. L.; Millan-Gabet, R.; Graham, J. R.; Hillenbrand, L. A.; Pott, J. U.; Ragland, S.; Wizinowich, P.
Language:English
Date of Publication (YYYY-MM-DD):2010
Title of Journal:The Astrophysical Journal
Journal Abbrev.:ApJ
Volume:718
Issue / Number:2
Start Page:774
End Page:794
Review Status:Peer-review
Audience:Experts Only
Abstract / Description:We present near-infrared observations of T Tauri and Herbig Ae/Be stars with a spatial resolution of a few milliarcseconds and a spectral resolution of ~2000. Our observations spatially resolve gas and dust in the inner regions of protoplanetary disks, and spectrally resolve broad-linewidth emission from the Brγ transition of hydrogen gas. We use the technique of spectro-astrometry to determine centroids of different velocity components of this gaseous emission at a precision orders of magnitude better than the angular resolution. In all sources, we find the gaseous emission to be more compact than or distributed on similar spatial scales to the dust emission. We attempt to fit the data with models including both dust and Brγ-emitting gas, and we consider both disk and infall/outflow morphologies for the gaseous matter. In most cases where we can distinguish between these two models, the data show a preference for infall/outflow models. In all cases, our data appear consistent with the presence of some gas at stellocentric radii of ~0.01 AU. Our findings support the hypothesis that Brγ emission generally traces magnetospherically driven accretion and/or outflows in young star/disk systems.
Free Keywords:circumstellar matter; stars: individual: AS 205 AS 353 DG Tau DK Tau DR Tau MWC 275 MWC 480 MWC 758 MWC 863 MWC 1080 RY Tau RW Aur V1057 Cyg V1331 Cyg V2508 Oph; stars: pre-main sequence; techniques: interferometric; techniques: spectroscopic
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2010ApJ...718..774E [ID No:1]
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