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Related papers: HD97048: a closer look to the disk

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We present high-contrast angular differential imaging (ADI) observations of the debris disk around HD 32297 in H-band, as well as the first polarimetric images for this system in polarized differential imaging (PDI) mode with Subaru/HICIAO.…

We present a direct imaging study of V892 Tau, a young Herbig Ae/Be star with a close-in stellar companion and circumbinary disk. Our observations consist of images acquired via Keck 2/NIRC2 with non-redundant masking and the pyramid…

Solar and Stellar Astrophysics · Physics 2023-10-17 Christina Vides , Steph Sallum , Josh Eisner , Andy Skemer , Ruth Murray-Clay

We present comprehensive models for the Herbig Ae stars MWC275 and AB Aur that aim to explain their spectral energy distribution (from UV to millimeter) and long baseline interferometry (from near-infrared to millimeter) simultaneously.…

HD50138 is a Herbig B[e] star with a circumstellar disc detected at IR and mm wavelength. Its brightness makes it a good candidate for NIR interferometry observations. We aim to resolve, spatially and spectrally, the continuum and hydrogen…

Solar and Stellar Astrophysics · Physics 2018-06-27 M. Koutoulaki , R. Garcia Lopez , A. Natta , A. Caratti o Garatti , D. Coffey , J. Sanchez-Bermudez , T. P. Ray

We present here $Spitzer$ mid-infrared (IR) spectra and modeling of the spectral energy distribution (SED) of a selection of post-Asymptotic Giant Branch (PAGB) stars. The mid-IR spectra of majority of these sources showed spectral features…

Solar and Stellar Astrophysics · Physics 2017-05-22 V. Venkata Raman , B. G. Anandarao , P. Janardhan , R. Pandey

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…

Solar and Stellar Astrophysics · Physics 2015-05-20 Göran Sandell , David A. Weintraub , Murad Hamidouche

Several arguments have been presented that favour a scenario in which the low detection rate of magnetic fields in Herbig Ae stars can be explained by the weakness of these fields and rather large measurement uncertainties.…

Solar and Stellar Astrophysics · Physics 2015-11-02 S. P. Järvinen , T. A. Carroll , S. Hubrig , M. Schöller , I. Ilyin , H. Korhonen , M. Pogodin , N. A. Drake

We attempt to constrain the physical properties of the inner, gaseous disk of the Herbig Be star BD+65 1637 using non-LTE, circumstellar disk codes and observed spectra (3700 to 10,500 \r{A}) from the ESPaDOnS instrument on CFHT. The…

Solar and Stellar Astrophysics · Physics 2016-01-27 P. Patel , T. A. A. Sigut , J. D. Landstreet

HD 179821 is an evolved star of unknown progenitor mass range (either post-Asymptotic Giant Branch or post-Red Supergiant) exhibiting a double peaked spectral energy distribution (SED) with a sharp rise from $\sim8-20$ $\mu$m. Such features…

HD~106906AB is so far the only young binary system around which a planet has been imaged and a debris disk evidenced thanks to a strong IR excess. As such, it represents a unique opportunity to study the dynamics of young planetary systems.…

We present diffraction-limited images in the 11.3 micron PAH band and in the continuum at 11.9 microns of the S287B star forming region obtained with the newly commissioned mid-infrared imager/spectrometer VISIR at the VLT. In both filters…

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

Aims. We present photometric data of debris disks around HIP 103389 (HD 199260), HIP 107350 (HN Peg, HD206860), and HIP 114948 (HD 219482), obtained in the context of our Herschel Open Time Key Program DUNES (DUst around NEarby Stars).…

The near-star environment around obscured stars is very dynamic. Many classes of stars show evidence for winds, disks, inflows and outflows with many phenomena occurring simultaneously. These processes are involved in stellar evolution,…

Astrophysics · Physics 2008-09-22 D. M. Harrington , J. R. Kuhn

Herbig Ae/Be stars are intermediate-mass pre-main sequence (PMS) stars showing signs of intense activity and strong stellar winds, whose origin is not yet understood in the frame of current theoretical models of stellar evolution for young…

Solar and Stellar Astrophysics · Physics 2015-05-30 Aurelie Fumel , Torsten Boehm

Context: Quantifying the gas content inside the dust gaps of transition disks is important to establish their origin. Aims: We seek to constrain the surface density of warm gas in the disk of HD 139614, a Herbig Ae star with a transition…

We present the first high-resolution X-ray spectrum of a prototypical Herbig star (AB Aurigae), measure and interpret various spectral features, and compare our results with model predictions. We use X-ray spectroscopy data from XMM-Newton.…

Astrophysics · Physics 2009-11-11 A. Telleschi , M. Guedel , K. R. Briggs , S. L. Skinner , M. Audard , E. Franciosini

We present new data of the protoplanetary disc surrounding the Herbig Ae/Be star HD 169142 obtained in the very broad-band (VBB) with the Zurich imaging polarimeter (ZIMPOL), a sub-system of the Spectro-Polarimetric High-contrast Exoplanet…

Earth and Planetary Astrophysics · Physics 2018-01-10 G. H. -M. Bertrang , H. Avenhaus , S. Casassus , M. Montesinos , F. Kirchschlager , S. Perez , L. Cieza , S. Wolf

We present the first ground-based near-infrared image of the circumstellar disk around the post-Herbig Ae/Be star HD141569A initially detected with the HST. Observations were carried out in the near-IR (2.2 $\mu$m) at the Palomar 200-inch…

Astrophysics · Physics 2008-11-26 A. Boccaletti , J. C. Augereau , F. Marchis , J. Hanh

We utilize a multi-step modelling process to produce synthetic interferometric and spectroscopic observables, which are then compared to their observed counterparts. Our extensive set of interferometric observations of the Be star 48 Per,…

Solar and Stellar Astrophysics · Physics 2017-07-05 C. E. Jones , T. A. A. Sigut , B. J. Grzenia , C. Tycner , R. T. Zavala

Herbig Ae/Be stars are young contracting stars on the radiative track in the HR diagram on their way to the main sequence. These stars provide a valuable link between high and low mass stars. Here we review the progress that has been made…

Solar and Stellar Astrophysics · Physics 2024-11-12 Sean D. Brittain , Inga Kamp , Gwendolyn Meeus , René D. Oudmaijer , L. B. F. M. Waters
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