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相关论文: The Circumstellar Environment of the TTS SU Auriga…

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SU Aurigae is a classical T Tauri star of spectral type G2. This star was one of the scientific targets of the MUSICOS 96 multi-site campaign that provided a wealth of high resolution cross-dispersed spectral data with a good continuous…

天体物理学 · 物理学 2007-05-23 J. M. Oliveira , B. H. Foing , Y. C. Unruh

We present a model of the circumstellar environment of the so-called ``Butterfly Star'' in Taurus (IRAS 04302+2247). The appearance of this young stellar object is dominated by a large circumstellar disk seen edge-on and the light…

天体物理学 · 物理学 2008-11-26 Sebastian Wolf , Deborah L. Padgett , Karl R. Stapelfeldt

The circumstellar environments of classical T Tauri stars are challenging to directly image because of their high star-to-disk contrast ratio. One method to overcome this is by using imaging polarimetry where scattered and consequently…

太阳与恒星天体物理 · 物理学 2015-06-17 S. V. Jeffers , M. Min , H. Canovas , M. Rodenhuis , C. U. Keller

SU Aurigae is a T Tauri star that was well monitored during the MUSICOS 96 multi-site campaign. We present the results of the spectroscopic analysis of the circumstellar environment of this star, particularly of the Halpha, Hbeta, Na I D…

天体物理学 · 物理学 2007-05-23 J. M. Oliveira , B. H. Foing , J. Th. van Loon , Y. C. Unruh

T Tauri stars are low-mass young stars whose disks provide the setting for planet formation. Despite this, their structure is poorly understood. We present new infrared interferometric observations of the SU Aurigae circumstellar…

SU Aurigae is a widely studied T Tauri star and here we present original state-of-the-art interferometric observations with better uv and baseline coverage than previous studies. We aim to investigate the characteristics of the…

We present mid-infrared spectra of T Tauri stars in the Taurus star-forming region obtained with the Spitzer Infrared Spectrograph (IRS). For the first time, the 5-36 micron spectra of a large sample of T Tauri stars belonging to the same…

The young star AB Aurigae is surrounded by a complex combination of gas-rich and dust dominated structures. The inner disk which has not been studied previously at sufficient resolution and imaging dynamic range seems to contain very little…

We study the inner region of the circumstellar disk around the TTauri star RY Tau. Our aim is to find a physical description satisfying the available interferometric data, obtained with the mid-infrared interferometric instrument at the…

天体物理学 · 物理学 2009-11-13 A. A. Schegerer , S. Wolf , Th. Ratzka , Ch. Leinert

We derive hydrostatic, radiative equilibrium models for passive disks surrounding T Tauri stars. Each disk is encased by an optically thin layer of superheated dust grains. This layer re-emits directly to space about half the stellar energy…

天体物理学 · 物理学 2009-06-16 E. I. Chiang , P. Goldreich

We review recent advances in our understanding of the innermost regions of the circumstellar environment around young stars, made possible by the technique of long baseline interferometry at infrared wavelengths. Near-infrared observations…

天体物理学 · 物理学 2007-05-23 Rafael Millan-Gabet , Fabien Malbet , Rachel Akeson , Christoph Leinert , John Monnier , Rens Waters

The combination of mid-infrared and recent submm/mm measurements allows us to set up the first comprehensive spectral energy distribution (SED) of the circumstellar material around a young Brown Dwarf. Simple arguments suggest that the dust…

天体物理学 · 物理学 2009-11-07 I. Pascucci , D. Apai , Th. Henning , C. P. Dullemond

We present mid-IR N-band $(\lambda_{eff} = 10.2\micron)$ photometry of a carefully selected sample of T Tauri stars thought to be single from the Taurus-Auriga molecular cloud. Infrared excesses in these stars are generally attributed to…

天体物理学 · 物理学 2008-11-26 Praveen Kundurthy , Michael R. Meyer , Massimo Robberto , Steven V. W. Beckwith , Tom Herbst

We present a spatially resolved 894 micron map of the circumstellar disk of the Butterfly star in Taurus (IRAS 04302+2247), obtained with the Submillimeter Array (SMA). The predicted and observed radial brightness profile agree well in the…

天体物理学 · 物理学 2009-11-13 S. Wolf , A. Schegerer , H. Beuther , D. L. Padgett , K. R. Stapelfeldt

We present our results from a mid-infrared interferometric survey targeted at the planet-forming region in the circumstellar disks around low- and intermediate-mass young stars. Our sample consist of 82 objects, including T Tauri stars,…

太阳与恒星天体物理 · 物理学 2020-02-14 J. Varga , P. Ábrahám , L. Chen , Th. Ratzka , K. É. Gabányi , Á. Kóspál

Investigating the evolution of protoplanetary disks is crucial for our understanding of star and planet formation. Several theoretical and observational studies have been performed in the last decades to advance this knowledge. FT Tauri is…

The inner 0.1 AU around accreting T Tauri stars hold clues to many physical processes that characterize the early evolution of solar-type stars. The accretion-ejection connection takes place at least in part in this compact magnetized…

天体物理学 · 物理学 2007-05-23 J. Bouvier , S. H. P. Alencar , T. J. Harries , C. M. Johns-Krull , M. M. Romanova

Birth environments of young stars have strong imprints on the star itself and their surroundings. We present a detailed analysis of the wealthy circumstellar environment around the young Herbig Ae/Be star TCrA. Our aim is to understand the…

We present the results of a 2.7 mm continuum interferometric survey of 24 young stellar objects in 11 fields. The target objects range from deeply embedded Class 0 sources to optical T Tauri sources. This is the first sub-arcsecond survey…

天体物理学 · 物理学 2009-10-12 Leslie W. Looney , Lee G. Mundy , W. J. Welch

We present high angular resolution observations with the Keck Interferometer, high dispersion spectroscopic observations with Keck/NIRSPEC, and near-IR photometric observations from PAIRITEL of a sample of 11 solar-type T Tauri stars in 9…

天体物理学 · 物理学 2009-11-13 J. A. Eisner , L. A. Hillenbrand , R. J. White , J. S. Bloom , R. L. Akeson , C. H. Blake
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