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相关论文: Resolved images of the protoplanetary disk around …

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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

We present recent near-infrared detections of circumstellar disks around the two old PMS Herbig stars HD 141569 and HD 100546 obtained with the HST/NICMOS2 camera. They reveal extended structures larger than 350-400 AU in radius. While the…

天体物理学 · 物理学 2007-05-23 J. C. Augereau , A. M. Lagrange , D. Mouillet , F. Menard

We investigate the physical properties and spatial distribution of Carbon Monoxide (CO) gas in the disks around the Herbig Ae/Be stars HD 97048 and HD 100546. Using high-spectral-resolution 4.588-4.715 $\mu$m spectra containing fundamental…

天体物理学 · 物理学 2015-05-13 G. van der Plas , M. E. van den Ancker , B. Acke , A. Carmona , C. Dominik , D. Fedele , L. B. F. M. Waters

Molecular line observations are powerful tracers of the physical and chemical conditions across the different evolutionary stages of star, disk and planet formation. Using the high angular resolution and unprecedented sensitivity of the…

地球与行星天体物理 · 物理学 2023-01-11 Alice S. Booth , John D. Ilee , Catherine Walsh , Mihkel Kama , Luke Keyte , Ewine F. van Dishoeck , Hideko Nomura

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

HD 163296 is one of the few protoplanetary discs displaying rings in the dust component. The present work uses ALMA observations of the 0.9 mm continuum emission having significantly better spatial resolution (~8 au) than previously…

太阳与恒星天体物理 · 物理学 2019-06-03 P. N. Diep , D. T. Hoai , N. B. Ngoc , P. T. Nhung , N. T. Phuong , T. T. Thai , P. Tuan-Anh

We investigate the structure and kinematics of the circumstellar disk around the Herbig Ae star MWC 758 using high resolution observations of the 12CO (3-2) and dust continuum emission at the wavelengths of 0.87 and 3.3 mm. We find that the…

太阳与恒星天体物理 · 物理学 2015-05-20 Andrea Isella , Antonella Natta , David Wilner , John M. Carpenter , Leonardo Testi

We report here the first resolved images of the circumstellar dust disk around the Pre-Main-Sequence star HD 100546. These near-infrared images were obtained in J and short K bands with the adaptive optics system ADONIS at the ESO…

天体物理学 · 物理学 2007-05-23 E. Pantin , C. Waelkens , P. O. Lagage

The disc around the Herbig Ae/Be star HD 100546 is one of the most extensively studied discs in the southern sky. Although there is a wealth of information about its dust content and composition, not much is known about its gas and large…

地球与行星天体物理 · 物理学 2015-05-18 O. Panić , E. F. van Dishoeck , M. R. Hogerheijde , A. Belloche , R. Güsten , W. Boland , A. Baryshev

We analyze a sample of 12 HST-selected edge-on protoplanetary disks for which the vertical extent of the emission layers can be constrained directly. We present ALMA high angular resolution continuum images (0.1arcsec) of these disks at two…

Gap-like structures in protoplanetary disks are likely related to planet formation processes. In this paper, we present and analyze high resolution (0.17*0.11 arcsec) 1.3 mm ALMA continuum observations of the protoplanetary disk around the…

We have investigated the spatial distribution, and the properties and chemical composition of the dust orbiting HD 100546. This system is remarkably different from other isolated Herbig Ae/Be stars in both the strength of the mid-IR excess…

天体物理学 · 物理学 2011-05-23 J. Bouwman , A. de Koter , C. Dominik , L. B. F. M Waters

HD100546 represents a particularly interesting target to study dynamical planet-disk interactions as various features have been observed in both the dust and gas that provide direct and indirect evidence for ongoing planet formation. In…

Circumstellar disks around stars older than 10 Myr are expected to be gas-poor. There are, however, two examples of old (30-40 Myr) debris-like disks containing a detectable amount of cold CO gas. Here we present ALMA and Herschel Space…

太阳与恒星天体物理 · 物理学 2015-06-17 A. Moór , A. Juhász , Á. Kóspál , P. Ábrahám , D. Apai , T. Csengeri , C. Grady , Th. Henning , A. M. Hughes , Cs. Kiss , I. Pascucci , M. Schmalzl , K. Gabányi

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 present preliminary results of spectroscopic data obtained with the La Silla 3.6m TIMMI2 and the VLT-ISAAC instruments. We have obtained 23 TIMMI2 N-band and 18 Q-band spectra for our total sample of 36 stars in March 2003 to investigate…

[Abridged] Far-infrared observations with Herschel revealed a surprisingly low abundance of cold-water reservoirs in protoplanetary discs. On the other hand, a handful of discs show emission of hot water transitions excited at temperatures…

地球与行星天体物理 · 物理学 2022-07-25 L. M. Pirovano , D. Fedele , E. F. van Dishoeck , M. R. Hogerheijde , G. Lodato , S. Bruderer

The formation of dust gaps in protoplanetary disks is one of the most important signposts of disk evolution and possibly the formation of planets. We aim to characterize the 'flaring' disk structure around the Herbig Ae/Be stars HD 100453…

太阳与恒星天体物理 · 物理学 2016-04-20 S. Khalafinejad , K. M. Maaskant , N. Marinas , A. G. G. M Tielens

In this paper, we analyse the upper limit fluxes of sub-millimeter ortho-H$_{2}$$^{16}$O 321 GHz, para-H$_{2}$$^{18}$O 322 GHz, and HDO 335 GHz lines from the protoplanetary disk around the Herbig Ae star HD 163296, using the Atacama Large…