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Related papers: PDS 144: The First Confirmed Herbig Ae - Herbig Ae…

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We present the first high angular resolution 1.4mm and 2.7mm continuum maps of the T Tauri binary system HK Tau obtained with the Plateau de Bure Interferometer. The contributions of both components are well disentangled at 1.4mm and the…

Astrophysics · Physics 2009-11-07 G. Duchene , F. Menard , K. Stapelfeldt , G. Duvert

Among the 21 Herbig Ae/Be stars studied, new detections of a magnetic field were achieved in six stars. For three Herbig Ae/Be stars, we confirm previous magnetic field detections. The largest longitudinal magnetic field, <B_z> = -454+-42G,…

Solar and Stellar Astrophysics · Physics 2015-05-13 S. Hubrig , B. Stelzer , M. Schoeller , C. Grady , O. Schuetz , M. A. Pogodin , M. Cure , K. Hamaguchi , R. V. Yudin

We report on the discovery of ETHOS 1 (PN G068.1+11.0), the first spectroscopically confirmed planetary nebula (PN) from a survey of the SuperCOSMOS Science Archive for high-latitude PNe. ETHOS 1 stands out as one of the few PNe to have…

Solar and Stellar Astrophysics · Physics 2015-05-20 B. Miszalski , R. L. M. Corradi , H. M. J. Boffin , D. Jones , L. Sabin , M. Santander-García , P. Rodríguez-Gil , M. M. Rubio-Díez

The Herbig Ae/Be star LkHalpha 101 has been imaged at high angular resolution at a number of wavelengths in the near-infrared (from 1 to 3 microns) using the Keck 1 Telescope, and also observed in the mid-infrared (11.15 microns) using the…

Astrophysics · Physics 2009-11-07 P. G. Tuthill , J. D. Monnier , W. C. Danchi , D. D. S. Hale , C. H. Townes

We present a study of the stellar parameters, distances and spectral energy distributions (SEDs) of HD 34282 and HD 141569, two pre-main sequence Herbig AeBe stars. Both objects have been reported to show `anomalous positions' in the HR…

Astrophysics · Physics 2009-11-10 B. Merín , B. Montesinos , C. Eiroa , E. Solano , A. Mora , P. D'Alessio , N. Calvet , EXPORT Collaboration

Our purpose is to study the effect of binary companions located within the first 10 stellar radii from the primary AGB star. In this work, we target the mass-losing carbon star V Hydrae (V Hya), looking for signatures of its companion in…

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…

Astrophysics · Physics 2009-11-11 B. Acke , M. E. van den Ancker

Measurements of gas mass in protoplanetary gas disks form the basis for estimating the conditions of planet formation. Among the most important constraints derived from disk diagnostics are the abundances of gas-phase species critical for…

Solar and Stellar Astrophysics · Physics 2021-04-14 P. Wilson Cauley , Kevin France , Gregory J. Herzceg , Christopher M. Johns-Krull

We have used the integral field spectrograph OSIRIS and laser guide star adaptive optics at Keck Observatory to obtain high angular resolution (0.06"), moderate spectral resolution (R ~ 3800) images of the bipolar jet from the Herbig Ae…

Astrophysics · Physics 2009-11-13 Marshall D. Perrin , James R. Graham

We report the first scattered light detection of a dusty debris disk surrounding the F2V star HD 15115 using the Hubble Space Telescope in the optical, and Keck adaptive optics in the near-infrared. The most remarkable property of the HD…

Astrophysics · Physics 2009-11-13 Paul Kalas , Michael P. Fitzgerald , James R. Graham

We obtained high angular resolution (~2") images of the 13CO(J=1-0) line and 2.7 millimeter continuum emission, and slightly lower resolution images of 12CO(J=1-0) and C18O(J=1-0) line emission toward the Herbig Ae star AB Aurigae. We…

Astrophysics · Physics 2009-11-10 Stuartt Corder , Josh Eisner , Anneila Sargent

We have carried out a survey of 60 Herbig Ae/Be stars in the 3 micron wavelength region in search for the rare spectral features at 3.43 and 3.53 micron. These features have been attributed to the presence of large, hot, hydrogen-terminated…

Astrophysics · Physics 2009-11-11 B. Acke , M. E. van den Ancker

Herbig Ae stars are young A-type stars in the pre-main sequence evolutionary phase with masses of ~1.5-3 M_o. They show rather intense surface activity (Dunkin et al. 1997) and infrared excess related to the presence of circumstellar disks.…

Astrophysics · Physics 2009-11-10 S. Hubrig , M. Schoeller , R. V. Yudin

A combination of high-resolution and wide-field imaging reveals two binary stars and one triple star system among the sample of the first 11 stars with planets detected by radial velocity variations. High resolution speckle or adaptive…

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…

Astrophysics · Physics 2009-11-11 Thomas Preibisch , Stefan Kraus , Thomas Driebe , Roy van Boekel , Gerd Weigelt

Active pre-main-sequence binaries with separations of around ten stellar radii present a wealth of phenomena unobserved in common systems. The study of these objects is extended from Classical T Tauri stars to the Herbig Ae star HD 104237.…

Solar and Stellar Astrophysics · Physics 2013-01-25 P. J. V. Garcia , M. Benisty , C. Dougados , F. Bacciotti , J. -M. Clausse , F. Massi , A. Mérand , R. Petrov , G. Weigelt

Deep HST broad-band images taken with ACS and WFPC2 of the giant ($\sim 1000$ AU diameter) dark silhouette proplyd 114-426 in the Orion Nebula show that this system is tilted, asymmetric, warped and photoevaporated. The exquisite angular…

Solar and Stellar Astrophysics · Physics 2016-03-02 Anna Miotello , Massimo Robberto , Marco A. C. Potenza , Luca Ricci

HR 4796A is surrounded by a well-structured and very bright circumstellar disc shaped like an annulus with many interesting features: very sharp inner and outer edges, brightness asymmetries, centre offset, and suspected distortions in the…

V921 Scorpii is a close binary system (separation 0.025") showing the B[e]-phenomenon. The system is surrounded by an enigmatic bipolar nebula, which might have been shaped by episodic mass-loss events, possibly triggered by dynamical…

Solar and Stellar Astrophysics · Physics 2015-06-04 Stefan Kraus , Nuria Calvet , Lee Hartmann , Karl-Heinz Hofmann , Alexander Kreplin , John D. Monnier , Gerd Weigelt

Herbig Ae/Be stars lie in the mass range between low and high mass young stars, and therefore offer a unique opportunity to observe any changes in the formation processes that may occur across this boundary. This paper presents medium…