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We present Subaru/HiCIAO H-band high-contrast images of the debris disk around HIP 79977, whose pres- ence was recently inferred from an infrared excess. Our images resolve the disk for the first time, allowing characterization of its…

We present Very Large Array observations at 7 mm that trace the thermal emission of large dust grains in the HD 169142 protoplanetary disk. Our images show a ring of enhanced emission of radius ~25-30 AU, whose inner region is devoid of…

We investigate high resolution imaging polarimetry of HD 169142 taken in the R' and I' bands with the SPHERE/ZIMPOL instrument for an accurate quantitative measurement of the radiation scattered by the circumstellar disk. We observe a…

Earth and Planetary Astrophysics · Physics 2021-11-10 C. Tschudi , H. M. Schmid

We present H-band VLT/NACO polarized light images of the Herbig Ae/Be star HD169142 probing its protoplanetary disk as close as ~0.1" to the star. Our images trace the face-on disk out to ~1.7" (~250 AU) and reveal distinct sub-structures…

Astrophysics of Galaxies · Physics 2015-06-15 Sascha P. Quanz , Henning Avenhaus , Esther Buenzli , Antonio Garufi , Hans Martin Schmid , Sebastian Wolf

In order to look for signs of on-going planet formation in young disks, we carried out the first J-band polarized emission imaging of the Herbig Ae/Be stars HD 150193, HD 163296, and HD 169142 using the Gemini Planet Imager (GPI), along…

We present high-contrast angular differential imaging (ADI) observations of the debris disk around HD 32297 in H-band, as well as the first polarimetric images for this system in polarized differential imaging (PDI) mode with Subaru/HICIAO.…

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…

We report Very Large Array observations at 7 mm, 9 mm, and 3 cm toward the pre-transitional disk of the Herbig Ae star HD 169142. These observations have allowed us to study the mm emission of this disk with the highest angular resolution…

The pre-transitional disk around the Herbig Ae star HD 169142 shows a complex structure of possible ongoing planet formation in dust thermal emission from the near infrared (IR) to millimeter wavelength range. Also, a distinct set of broad…

Solar and Stellar Astrophysics · Physics 2016-02-17 Ji Yeon Seok , Aigen Li

Debris disks or belts are important signposts for the presence of colliding planetesimals and, therefore, for ongoing planet formation and evolution processes in young planetary systems. Imaging of debris material at small separations from…

Earth and Planetary Astrophysics · Physics 2018-10-24 N. Engler , H. M. Schmid , S. P. Quanz , H. Avenhaus , A. Bazzon

HD$\,$169142 is an excellent target to investigate signs of planet-disk interaction due to the previous evidence of gap structures. We performed J-band (~1.2{\mu}m) polarized intensity imaging of HD169142 with VLT/SPHERE. We observe…

The protoplanetary system HD 169142 is one of the few cases where a potential candidate protoplanet has been recently detected via direct imaging. To study the interaction between the protoplanet and the disk itself observations of the gas…

Solar and Stellar Astrophysics · Physics 2017-04-05 D. Fedele , M. Carney , M. R. Hogerheijde , C. Walsh , A. Miotello , P. Klaassen , S. Bruderer , Th. Henning , E. F. vanDishoeck

We present new data of the protoplanetary disc surrounding the Herbig Ae/Be star HD 169142 obtained in the very broad-band (VBB) with the Zurich imaging polarimeter (ZIMPOL), a sub-system of the Spectro-Polarimetric High-contrast Exoplanet…

Earth and Planetary Astrophysics · Physics 2018-01-10 G. H. -M. Bertrang , H. Avenhaus , S. Casassus , M. Montesinos , F. Kirchschlager , S. Perez , L. Cieza , S. Wolf

We present H- and Ks-band polarized differential images (PDI) of the Herbig Ae/Be star HD142527, revealing its optically thick outer disk and the nearly empty gap. The very small inner working angle (~0.1") and high resolution achievable…

Solar and Stellar Astrophysics · Physics 2015-06-18 Henning Avenhaus , Sascha P. Quanz , Hans Martin Schmid , Michael R. Meyer , Antonio Garufi , Sebastian Wolf , Carsten Dominik
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