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Related papers: Polarization of Herbig Ae/Be candidates and their …

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Inner regions of protoplanetary disks host many complex physical processes such as star-disk interactions, magnetic fields, planet formation, and the migration of new planets. To directly study this region requires milli-arcsecond angular…

Our knowledge of the presence and the role of magnetic fields in intermediate-mass pre-main-sequence stars remains very poor. We present the magnetic properties of four Herbig Ae/Be stars that have not been previously studied in detail. Our…

Solar and Stellar Astrophysics · Physics 2015-06-03 S. Hubrig , M. Schoeller , I. Ilyin , C. R. Cowley , Z. Mikulasek , B. Stelzer , M. A. Pogodin , R. V. Yudin , M. Cure

We present near-IR (J,H,Ks) photometry for 27 of the 28 candidate Herbig Ae/Be stars in the Small and Large Magellanic Clouds identified via the EROS1 and EROS2 surveys as well as near-contemporaneous optical (H-alpha) spectroscopy for 21…

Solar and Stellar Astrophysics · Physics 2015-05-28 Bradley W. Rush , John P. Wisniewski , Karen S. Bjorkman

We seek to find the precursors of the Herbig Ae/Be stars in the solar vicinity within 500 pc from the Sun. We do this by creating an optically selected sample of intermediate mass T-Tauri stars (IMTT stars) here defined as stars of masses…

Solar and Stellar Astrophysics · Physics 2021-08-25 P. G. Valegård , L. B. F. M. Waters , C. Dominik

W5-E has been observed with the Herschel-PACS and -SPIRE photometers, at 100, 160, 250, 350, and 500 microns. The dust temperature map shows a rather uniform temperature, in the range 17.5-20 K in the dense condensations or filaments, 21-22…

Astrophysics of Galaxies · Physics 2015-06-11 L. Deharveng , A. Zavagno , L. D. Anderson , F. Motte , A. Abergel , Ph. Andre , S. Bontemps , G. Leleu , H. Roussel , D. Russeil

Using high-resolution data from the Galactic Arecibo L-Band Feed Array HI (GALFA-HI) survey, we show that linear structure in Galactic neutral hydrogen (HI) correlates with the magnetic field orientation implied by Planck 353 GHz polarized…

Cosmology and Nongalactic Astrophysics · Physics 2015-12-16 S. E. Clark , J. Colin Hill , J. E. G. Peek , M. E. Putman , B. L. Babler

We studied a small comet-shape reflection nebula, located in the dark cloud SL 4 in the Vela Molecular Ridge cloud C, known as BBWo 192E (GM 1-23), and a young infrared cluster embedded into the nebula, for the evidences of recent star…

Solar and Stellar Astrophysics · Physics 2020-10-07 T. Yu. Magakian , T. A. Movsessian , H. R. Andreasyan , J. Bally , A. S. Rastorguev

We have found Herbig Ae/Be star candidates in the western region of the Magellanic Bridge. Using the near infrared camera SIRIUS and the 1.4 m telescope IRSF, we surveyed about 3.0 deg x 1.3 deg (24 deg < RA < 36 deg, -75 deg < Dec. < -73.7…

Cross-correlation of the DIRBE 100 micron survey with previously published H-alpha maps tests correlations between far-infrared dust and the warm ionized interstellar medium in different regions of the sky. A 10 x 12 deg patch at Galactic…

Astrophysics · Physics 2009-10-30 A. Kogut

We investigate variations in the linear polarization as well as in the V-band and B-band colour-magnitudes for classical Be star disks. We present two models: disks with enhanced disk density and disks that are tilted or warped from the…

Solar and Stellar Astrophysics · Physics 2018-03-28 Keegan C. Marr , C. E. Jones , R. J. Halonen

We have obtained linear polarization measurements of the Large Magellanic Cloud B[e] supergiant S 111 using optical imaging polarimetry. The intrinsic polarization found is consistent with the presence of an axisymmetric circumstellar…

Astrophysics · Physics 2009-11-07 R. Melgarejo , A. M. Magalhaes , A. C. Carciofi , C. V. Rodrigues

We use the long-slit spectroscopy mode of the VISIR-NEAR experiment to perform diffraction-limited observations of eight nearby Herbig Ae protoplanetary disks. We extract spectra for various locations along the slit with a spectral…

We have conducted a high signal-to-noise spectroscopic survey of 670 nearby early-type stars, to map Diffuse Interstellar Band (DIB) absorption in and around the Local Bubble. The project started with a Southern hemisphere survey conducted…

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…

We present a comprehensive mid-infrared spectroscopic survey of 124 Herbig Ae/Be stars using newly processed Spitzer/IRS spectra from the newly released CASSISjuice database. Based on prominent dust and molecular signatures (polycyclic…

Solar and Stellar Astrophysics · Physics 2025-06-18 R. Arun , Blesson Mathew , B. Shridharan , K. Ujjwal , Akhil Krishna R , G. Maheswar , Sreeja S. Kartha

The structure of the dusty circumstellar envelopes (CSEs) of proto-planetary nebulae (PPNs) reveals the mass-loss history of these sources and how such histories may differ for elliptical (SOLE) and bipolar (DUPLEX) PPNs. To study the PPN…

Astrophysics · Physics 2008-11-26 Toshiya Ueta , Koji Murakawa , Margaret Meixner

Stellar population and the interstellar gas-dust medium in the vicinity of the open star cluster vdB 130 are analysed using optical observations taken with the 6-m telescope of the SAO RAS and the 125-cm telescope of the SAI MSU along with…

We present optical and millimetric data for 47 intermediate Hubble type spiral galaxies located either in dense environments or in the field. We compare correlations between global parameters, such as far-infrared luminosity, blue…

Astrophysics · Physics 2009-11-07 Duilia F. de Mello , Marcio A. G. Maia , Tommy Wiklind

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…

We have observed 14 Herbig Ae/Be sources with the long-baseline near-IR Palomar Testbed Interferometer, All except two sources are resolved at 2.2 um, with angular sizes generally <5 mas. We determine the size scales and orientations of the…

Astrophysics · Physics 2009-11-10 J. A. Eisner , B. F. Lane , L. A. Hillenbrand , R. L. Akeson , A. I. Sargent
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