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相关论文: First evidence for dusty disks around Herbig Be st…

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We completed a search for circumstellar disks around Herbig Be stars using the NRAO Very Large Array (VLA) and the IRAM Plateau de Bure (PdB) interferometers. We present our new VLA and PdBI data for the three objects MWC 297, Z CMa, and…

天体物理学 · 物理学 2009-11-13 T. Alonso-Albi , A. Fuente , R. Bachiller , R. Neri , P. Planesas , L. Testi , O. Berne , C. Joblin

We present high-angular resolution observations of the circumstellar disk around the massive Herbig Be star R Mon (M~8 Msun) in the continuum at 2.7mm and 1.3mm and the CO 1->0 and 2->1 rotational lines. Based on the new 1.3mm continuum…

广义相对论与量子宇宙学 · 物理学 2011-02-11 A. Fuente , T. Alonso-Albi , R. Bachiller , A. Natta , L. Testi , R. Neri , P. Planesas

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

The recent findings of gas giant planets around young A-type stars suggest that disks surrounding Herbig Ae/Be stars will develop planetary systems. An interesting case is HD142527, for which previous observations revealed a complex…

We present high-spectral-resolution, optical spectra of the Herbig Be star MWC 147, in which we spectrally resolve several emission lines, including the [O I] lines at 6300 and 6363\deg. Their highly symmetric, double-peaked line profiles…

地球与行星天体物理 · 物理学 2015-05-20 T. Bagnoli , R. van Lieshout , L. B. F. M. Waters , G. van der Plas , B. Acke , H. van Winckel , G. Raskin , P. D. Meerburg

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

Herbig Ae stars (HAe) are the precursors of Vega-type systems and, therefore, crucial objects in planet formation studies. Thus far, only a few disks associated with HAe stars have been studied using millimetre interferometers. Our aim is…

太阳与恒星天体物理 · 物理学 2015-05-28 Jeremie Boissier , Tomas Alonso-Albi , Asuncion Fuente , Olivier Berne , Rafael Bachiller , Roberto Neri , David Ginard

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…

We present high resolution 0.45" x 0.32" observations from the BIMA array toward the Herbig Ae system MWC 480 in the lambda = 1.4 mm dust continuum. We resolve a circumstellar disk of radius ~170 AU and constrain the disk parameters by…

天体物理学 · 物理学 2008-11-26 Murad Hamidouche , Leslie W. Looney , Lee G. Mundy

We present new multi-wavelength millimeter interferometric observations of the Herbig Ae star HD 163296 obtained with the IRAM/PBI, SMA and VLA arrays both in continuum and in the 12CO, 13CO and C18O emission lines. Gas and dust properties…

天体物理学 · 物理学 2009-11-13 A. Isella , L. Testi , A. Natta , R. Neri , D. Wilner , C. Qi

In this Paper we present high angular resolution imaging of 3 intermediate-mass (IM) stars using the Plateau de Bure Interferometer (PdBI). In particular we present the chemical study we have carried out towards the IM hot core NGC…

天体物理学 · 物理学 2009-06-23 A. Fuente

We present observations of six isolated, pre-main-sequence, intermediate mass stars selected for shallow spectra at submillimeter wavelengths at 1.3, 2.6, 7.0, and 36 millimeters from the IRAM PdBI and the VLA. We analyze the new…

天体物理学 · 物理学 2009-11-10 A. Natta , L. Testi , R. Neri , D. S. Shepherd , D. J. Wilner

We have acquired sub-millimeter observations of 33 fields containing 37 Herbig Ae/Be (HAEBE) stars or potential HAEBE stars, including SCUBA maps of all but two of these stars. Nine target stars show extended dust emission. The other 18 are…

太阳与恒星天体物理 · 物理学 2015-05-20 Göran Sandell , David A. Weintraub , Murad Hamidouche

We present 7 mm and 3.5 cm wavelength continuum observations toward the Herbig AeBe star HD169142 performed with the Very Large Array (VLA) with an angular resolution of ~1". We find that this object exhibits strong (~4.4 mJy), unresolved…

天体物理学 · 物理学 2016-08-16 W. R. F. Dent , J. M. Torrelles , M. Osorio , N. Calvet , G. Anglada

We present subarcsecond observations at 2.7 and 1.4 mm of a sample of massive young stellar objects made with the BIMA millimetre array. For most sources the continuum emission on the smallest scales at 2.7 mm is dominated by free-free…

天体物理学 · 物理学 2007-05-23 Andy Gibb , Melvin Hoare , Lee Mundy , Friedrich Wyrowski

We have used mid-infrared long-baseline interferometry with MIDI at the VLTI to resolve the circumstellar material around the Herbig Ae star HR 5999, providing the first direct measurement of its angular size, and to derive constraints on…

天体物理学 · 物理学 2009-11-11 Thomas Preibisch , Stefan Kraus , Thomas Driebe , Roy van Boekel , Gerd Weigelt

Context. It is now generally accepted that the near-infrared excess of Herbig AeBe stars originates in the dust of a circumstellar disk. Aims. The aims of this article are to infer the radial and vertical structure of these disks at scales…

We present the results of the interferometric observations of the circumstellar disk surrounding MWC 297 in the continuum at 230 GHz (1.3 mm) and in the (J=2-1) rotational transitions of $^{12}$CO,$^{13}$CO and C$^{18}$O using the…

天体物理学 · 物理学 2009-11-13 P. Manoj , Paul T. P. Ho , Nagayoshi Ohashi , Qizhou Zhang , T. Hasegawa , Huei-Ru Chen , H. C. Bhatt , N. M. Ashok

We report the results of a sensitive K-band survey of Herbig Ae/Be disk sizes using the 85-m baseline Keck Interferometer. Targets were chosen to span the maximum range of stellar properties to probe the disk size dependence on luminosity…

Circumstellar discs are essential for high mass star formation, while multiplicity, in particular binarity, appears to be an inevitable outcome since the vast majority of massive stars (> 8 Msun) are found in binaries (up to 100%). We…

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