English
Related papers

Related papers: Sparse Aperture Masking Observations of the FL Cha…

200 papers

The transition disk around the T Tauri star T Cha possesses a large gap, making it a prime target for high-resolution imaging in the context of planet formation. We aim to find signs of disk evolutionary processes by studying the disk…

With the uniquely high contrast within 0.1" (\Delta mag(L') = 5-6.5 magnitudes) available using Sparse Aperture Masking (SAM) with NACO at VLT, we detected asymmetry in the flux from the Herbig Fe star HD 142527 with a barycenter emission…

(Abridged) Circumstellar disks are believed to be the birthplace of planets and are expected to dissipate on a timescale of a few Myr. The processes responsible for the removal of the dust and gas will strongly modify the radial…

Recently, analysis of near-infrared broad-band photometry and Spitzer IRS spectra has led to the identification of a new "pre-transitional disk" class whose members have an inner optically thick disk separated from an outer optically thick…

Young circumstellar disks are of prime interest to understand the physical and chemical conditions under which planet formation takes place. Only very few detections of planet candidates within these disks exist, and most of them are…

Earth and Planetary Astrophysics · Physics 2018-09-12 M. Keppler , M. Benisty , A. Müller , Th. Henning , R. van Boekel , F. Cantalloube , C. Ginski , R. G. van Holstein , A. -L. Maire , A. Pohl , M. Samland , H. Avenhaus , J. -L. Baudino , A. Boccaletti , J. de Boer , M. Bonnefoy , G. Chauvin , S. Desidera , M. Langlois , C. Lazzoni , G. Marleau , C. Mordasini , N. Pawellek , T. Stolker , A. Vigan , A. Zurlo , T. Birnstiel , W. Brandner , M. Feldt , M. Flock , J. Girard , R. Gratton , J. Hagelberg , A. Isella , M. Janson , A. Juhasz , J. Kemmer , Q. Kral , A. -M. Lagrange , R. Launhardt , A. Matter , F. Ménard , J. Milli , P. Mollière , J. Olofsson , L. Perez , P. Pinilla , C. Pinte , S. P. Quanz , T. Schmidt , S. Udry , Z. Wahhaj , J. P. Williams , E. Buenzli , M. Cudel , C. Dominik , R. Galicher , M. Kasper , J. Lannier , D. Mesa , D. Mouillet , S. Peretti , C. Perrot , G. Salter , E. Sissa , F. Wildi , L. Abe , J. Antichi , J. -C. Augereau , A. Baruffolo , P. Baudoz , A. Bazzon , J. -L. Beuzit , P. Blanchard , S. S. Brems , T. Buey , V. De Caprio , M. Carbillet , M. Carle , E. Cascone , A. Cheetham , R. Claudi , A. Costille , A. Delboulbé , K. Dohlen , D. Fantinel , P. Feautrier , T. Fusco , E. Giro , D. Gisler , L. Gluck , C. Gry , N. Hubin , E. Hugot , M. Jaquet , D. Le Mignant , M. Llored , F. Madec , Y. Magnard , P. Martinez , D. Maurel , M. Meyer , O. Moeller-Nilsson , T. Moulin , L. Mugnier , A. Origne , A. Pavlov , D. Perret , C. Petit , J. Pragt , P. Puget , P. Rabou , J. Ramos , F. Rigal , S. Rochat , R. Roelfsema , G. Rousset , A. Roux , B. Salasnich , J. -F. Sauvage , A. Sevin , C. Soenke , E. Stadler , M. Suarez , M. Turatto , L. Weber

Stellar coronagraph performance is highly sensitive to optical aberrations. In order to effectively suppress starlight for exoplanet imaging applications, low-order wavefront aberrations entering a coronagraph such as tip-tilt, defocus and…

Instrumentation and Methods for Astrophysics · Physics 2015-06-17 Hari Subedi , Neil T. Zimmerman , N. Jeremy Kasdin , Kathleen Cavanagh , A J Eldorado Riggs

We re-analyze VLT/SPHERE-IRDIS K and H-band sparse aperture masking interferometry data of the transition disk HD 100546 observed in 2018 and 2021, respectively. We fit geometrical models to the closure phases extracted from both datasets.…

Transition disks with small inner dust cavities are interesting targets for the study of disk clearing mechanisms. Such disks have been identified through a deficit in the infrared part of their SED, but spatially resolved millimeter…

Mid-infrared spectrophotometric observations have revealed a small sub-class of circumstellar disks with spectral energy distributions (SEDs) suggestive of large inner gaps with low dust content. However, such data provide only an indirect…

Astrophysics · Physics 2009-10-02 J. M Brown , G. A. Blake , C. Qi , C. P. Dullemond , D. J. Wilner

The transition between massive Class II circumstellar disks and Class III debris disks, with dust residuals, has not yet been clearly understood. Disks are expected to dissipate with time, and dust clearing in the inner regions can be the…

Transition disks are protoplanetary disks with inner cavities possibly cleared by massive companions, which makes them prime targets to observe at high resolution to map their velocity structure. We present ALMA Band 6 dust and gas…

It has been suggested that the gaps and cavities recently discovered in transitional disks are opened by planets. To explore this scenario, we combine two-dimensional two fluid (gas + particle) hydrodynamical calculations with…

Earth and Planetary Astrophysics · Physics 2015-08-19 Ruobing Dong , Zhaohuan Zhu , Barbara Whitney

With an emphasis on improving the fidelity even in super-resolution regimes, new imaging techniques have been intensively developed over the last several years, which may provide substantial improvements to the interferometric observation…

The recently recognized class of "transitional disk" systems consists of young starswith optically-thick outer disks but inner disks which are mostly devoid of small dust. Here we introduce a further class of "pre-transitional disks" with…

Astrophysics · Physics 2009-11-13 C. Espaillat , N. Calvet , P. D'Alessio , J. Hernandez , C. Qi , L. Hartmann , E. Furlan , D. M. Watson

MICADO, the European Extremely Large Telescope first light imager will feature a dedicated high contrast imaging mode specifically designed for observing and characterizing exoplanets and circumstellar disks. Two sparse aperture masks (SAM)…

Instrumentation and Methods for Astrophysics · Physics 2024-09-02 Elsa Huby , Pierre Baudoz , Sylvestre Lacour , Manon Le Teuff , Yann Clénet , Richard Davies

Transitional disks are protoplanetary disks characterized by reduced near- and mid-infrared emission with respect to full disks. This characteristic spectral energy distribution indicates the presence of an optically thin inner cavity…

Earth and Planetary Astrophysics · Physics 2015-06-19 J. T. Keane , I. Pascucci , C. Espaillat , P. Woitke , S. Andrews , I. Kamp , W. -F. Thi , G. Meeus , W. R. F. Dent

In this study, we reported the results of high-resolution (0.14 arcsec) Atacama Large Millimeter/submillimeter Array (ALMA) observations of the 225 GHz dust continuum and CO molecular emission lines from the transitional disk around SY Cha.…