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相关论文: Resolving structure of the disk around HD100546 at…

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We present mid-infrared nulling interferometric and direct imaging observations of the Herbig Ae star HD 100546 obtained with the Magellan I (Baade) 6.5 m telescope. The observations show resolved circumstellar emission at 10.3, 11.7, 12.5,…

天体物理学 · 物理学 2009-11-10 W. M. Liu , P. M. Hinz , M. R. Meyer , E. E. Mamajek , W. F. Hoffmann , J. L. Hora

The disk around the Herbig Ae/Be star HD 100546 has been extensively studied and it is one of the systems for which there are observational indications of ongoing and/or recent planet formation. However, up until now no resolved image of…

太阳与恒星天体物理 · 物理学 2015-06-19 Jaime E. Pineda , Sascha P. Quanz , Farzana Meru , Gijs D. Mulders , Michael R. Meyer , Olja Panić , Henning Avenhaus

Studying the physical conditions in circumstellar disks is a crucial step toward understanding planet formation. Of particular interest is the case of HD 100546, a Herbig Be star that presents a gap within the first 13 AU of its…

太阳与恒星天体物理 · 物理学 2015-05-27 E. Tatulli , M. Benisty , F. Ménard , P. Varnière , C. Martin-Zaidi , W. -F. Thi , C. Pinte , F. Massi , G. Weigelt , K. -H. Hofmann , R. G. Petrov

We present high-contrast observations of the circumstellar environment of the Herbig Ae/Be star HD100546. The final 3.8 micron image reveals an emission source at a projected separation of 0.48"+-0.04" (corresponding to ~47+-4 AU at a…

星系天体物理 · 物理学 2015-06-15 Sascha P. Quanz , Adam Amara , Michael R. Meyer , Matthew A. Kenworthy , Markus Kasper , Julien H. Girard

We present the first multi-wavelength, high-contrast imaging study confirming the protoplanet embedded in the disk around the Herbig Ae/Be star HD100546. The object is detected at $L'$ ($\sim 3.8\,\mu m$) and $M'$ ($\sim 4.8\,\mu m$), but…

太阳与恒星天体物理 · 物理学 2015-04-16 Sascha P. Quanz , Adam Amara , Michael R. Meyer , Julien H. Girard , Matthew A. Kenworthy , Markus Kasper

Disclosing the structure of disks surrounding Herbig AeBe stars is important to expand our understanding of the formation and early evolution of stars and planets. We aim at revealing the sub-AU disk structure around the 10 Myr old Herbig…

太阳与恒星天体物理 · 物理学 2015-05-18 M. Benisty , E. Tatulli , F. Menard , M. Swain

HD 100546 is a well-studied Herbig Be star-disk system that likely hosts a close-in companion with compelling observational evidence for an embedded protoplanet at 68 AU. We present ALMA observations of the HD 100546 disk which resolve the…

We present long baseline Atacama Large Millimeter/submillimeter Array (ALMA) observations of the 870$\,\mu$m dust continuum emission and CO (3-2) from the protoplanetary disk around the Herbig Ae/Be star HD 100546, which is one of the few…

太阳与恒星天体物理 · 物理学 2019-01-30 J. E. Pineda , J. Szulágyi , S. P. Quanz , E. F. van Dishoeck , A. Garufi , F. Meru , G. D. Mulders , L. Testi , M. R. Meyer , M. Reggiani

Aims. We intend to spatially and spectrally resolve the [O I] emission region in two nearby Herbig stars. Methods. We present high-resolution (R = 80,000) VLT/UVES echelle spectra of the [O I] 6300A line in the Herbig Ae/Be stars HD 97048…

天体物理学 · 物理学 2009-11-11 B. Acke , M. E. van den Ancker

Coronagraphic imaging with the Near Infrared Camera and Multi Object Spectrometer on the Hubble Space Telescope reveals a large, ~400 AU (4'') radius, circumstellar disk around the Herbig Ae/Be star HD 141569. A reflected light image at 1.1…

Context. The protoplanetary disk around the star HD 100546 displays prominent substructures in the form of two concentric rings. Recent observations with the Atacama Large Millimeter/sub-millimeter Array (ALMA) have revealed these features…

地球与行星天体物理 · 物理学 2021-12-22 Max Ackermann Pyerin , Timmy N. Delage , Nicolás T. Kurtovic , Matías Gárate , Thomas Henning , Paola Pinilla

The disk atmosphere is one of the fundamental elements of theoretical models of a protoplanetary disk. However, the direct observation of the warm gas (>> 100 K) at large radius of a disk (>> 10 AU) is challenging, because the line emission…

星系天体物理 · 物理学 2015-06-03 M. Goto , G. van der Plas , M. van den Ancker , C. P. Dullemond , A. Carmona , Th. Henning , G. Meeus , H. Linz , B. Stecklum

A region of roughly half of the solar system scale around the star HD 100546 is largely cleared of gas and dust, in contrast to the bright outer disc. However, some material is observed in the immediate vicinity of the star. We investigate…

地球与行星天体物理 · 物理学 2015-06-04 O. Panic , Th. Ratzka , G. D. Mulders , C. Dominik , R. van Boekel , Th. Henning , W. Jaffe , M. Min

HD 100546 is one of the few known pre-main-sequence stars that may host a planetary system in its disk. We analyze new VLT/SPHERE/ZIMPOL polarimetric images of HD 100546 with filters in H$\alpha$ and the adjacent continuum. We have probed…

太阳与恒星天体物理 · 物理学 2017-12-13 I. Mendigutía , R. D. Oudmaijer , A. Garufi , S. L. Lumsden , N. Huélamo , A. Cheetham , W. J. de Wit , B. Norris , F. A. Olguin , P. Tuthill

We report high-resolution 1.6 $\micron$ polarized intensity ($PI$) images of the circumstellar disk around the Herbig Ae star AB Aur at a radial distance of 22 AU ($0."15$) up to 554 AU (3.$"$85), which have been obtained by the…

Spatially resolving the inner dust cavity of the transitional disks is a key to understanding the connection between planetary formation and disk dispersal. The disk around the Herbig star HD 139614 is of particular interest since it…

地球与行星天体物理 · 物理学 2016-01-20 A. Matter , L. Labadie , J. -C. Augereau , J. Kluska , A. Crida , A. Carmona , J. F. Gonzalez , W. F. Thi , J. -B. Le Bouquin , J. Olofsson , B. Lopez

Protoplanetary disks around young stars harbor many structures related to planetary formation. Of particular interest, spiral patterns were discovered among several of these disks and are expected to be the sign of gravitational…

地球与行星天体物理 · 物理学 2015-06-17 A. Boccaletti , E. Pantin , A. -M. Lagrange , J. -C. Augereau , H. Meheut , S. P. Quanz

We present polarimetric differential imaging (PDI) data of the circumstellar disk around the Herbig Ae/Be star HD100546 obtained with VLT/NACO. We resolve the disk in polarized light in the H and Ks filter between ~0.1-1.4" (i.e., ~10-140…

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