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相关论文: The inner structure of the TW Hya Disk as revealed…

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We present a 0.5-2.2 micron scattered light spectrum of the circumstellar disk around TW Hya from a combination of spatially resolved HST STIS spectroscopy and NICMOS coronagraphic images of the disk. We investigate the morphology of the…

地球与行星天体物理 · 物理学 2015-06-16 J. H. Debes , H. Jang-Condell , A. J. Weinberger , A. Roberge , G. Schneider

We report new total intensity visible light high contrast imaging of the TW Hya disk taken with the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope (HST). This represents the first published images of the disk with…

太阳与恒星天体物理 · 物理学 2023-05-08 J. Debes , R. Nealon , R. Alexander , A. J. Weinberger , S. G. Wolff , D. Hines , J. Kastner , H. Jang-Condell , C. Pinte , P. Plavchan , L. Pueyo

The face-on disk around TW Hya is imaged in scattered light at wavelengths of 1.1 and 1.6 micron using the coronagraph in the Near Infrared Camera and Multi Object Spectrometer aboard the Hubble Space Telescope. Stellar light scattered from…

We have obtained new images of the protoplanetary disk orbiting TW Hya in visible, total intensity light with the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope (HST), using the newly commissioned BAR5 occulter.…

We present a new Subaru/HiCIAO high-contrast H-band polarized intensity (PI) image of a nearby transitional disk associated with TW Hydrae. The scattered light from the disk was detected from 0.2" to 1.5" (11 - 81 AU) and the PI image shows…

Context. Some of transition disks show asymmetric structures in thermal sub-millimetre emission and optical scattered light. These structures can be the result of planet(s) or companions embedded in the disk. Aims. We aim to detect and…

地球与行星天体物理 · 物理学 2015-11-18 P. Pinilla , J. de Boer , M. Benisty , A. Juhász , M. de Juan Ovelar , C. Dominik , H. Avenhaus , T. Birnstiel , J. H. Girard , N. Huelamo , A. Isella , J. Milli

Three-dimensional hydrodynamic numerical simulations have demonstrated that the structure of a protoplanetary disc may be strongly affected by a planet orbiting in a plane that is misaligned to the disc. When the planet is able to open a…

地球与行星天体物理 · 物理学 2019-02-13 Rebecca Nealon , Christophe Pinte , Richard Alexander , Daniel Mentiplay , Giovanni Dipierro

We present scattered light images of the TW Hya disk performed with SPHERE in PDI mode at 0.63, 0.79, 1.24 and 1.62 micron. We also present H2/H3-band ADI observations. Three distinct radial depressions in the polarized intensity…

We have obtained Hubble Space Telescope (HST) coronagraphic observations of the circumstellar disk around M star TWA 7 using the STIS instrument in visible light. Together with archival observations including HST/NICMOS using the F160W…

We present the first spatially resolved spectrum of scattered light from the TW Hydrae protoplanetary disk. This nearly face-on disk is optically thick, surrounding a classical T Tauri star in the nearby 10 Myr old TW Hya association. The…

天体物理学 · 物理学 2009-11-10 Aki Roberge , Alycia J. Weinberger , Eliot M. Malumuth

We test the hypothesis that the sub-millimetre thermal emission and scattered light gaps seen in recent observations of TW Hya are caused by planet-disc interactions. We perform global three-dimensional dusty smoothed particle hydrodynamics…

地球与行星天体物理 · 物理学 2018-11-12 Daniel Mentiplay , Daniel J. Price , Christophe Pinte

We examine the observational appearance of partial gaps being opened by planets in protoplanetary disks, considering the effects of the inclination relative to the line of sight. The gap's trough is darkened by both shadowing and cooling,…

地球与行星天体物理 · 物理学 2015-06-16 Hannah Jang-Condell , Neal J. Turner

We present ALMA Cycle~2 observations at $0.5^{\prime\prime}$ resolution of TW Hya of CS $J=5-4$ emission. The radial profile of the integrated line emission displays oscillatory features outwards of $1.5^{\prime\prime}$ ($\approx 90$ au). A…

地球与行星天体物理 · 物理学 2017-02-09 R Teague , D Semenov , U Gorti , S Guilloteau , Th. Henning , T. Birnstiel , A. Dutrey , R. van Boekel , E. Chapillon

We analyze high angular resolution ALMA observations of the TW Hya disk to place constraints on the CO and dust properties. We present new, sensitive observations of the $^{12}$CO $J = 3-2$ line at a spatial resolution of 8 AU (0\farcs14).…

We report the discovery of a scattering component around the HD 141569 A circumstellar debris system, interior to the previously known inner ring. The discovered inner disk component, obtained in broadband optical light with HST/STIS…

We present Hubble Space Telescope Near-Infrared Camera and Multi-Object Spectrometer coronagraphic imaging polarimetry of the TW Hydrae protoplanetary disk. These observations simultaneously measure the total and polarized intensity,…

We present H and K band imaging polarimetry for the PDS 66 circumstellar disk obtained during the commissioning of the Gemini Planet Imager (GPI). Polarization images reveal a clear detection of the disk in to the 0.12'' inner working angle…

We fit an isothermal oscillatory density model to the outer disk of TW Hya in which planets have presumably already formed and they are orbiting within four observed dark gaps. At first sight, this 52 AU small disk does not appear to be…

地球与行星天体物理 · 物理学 2019-03-05 Dimitris M. Christodoulou , Demosthenes Kazanas
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