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The QSO HE0450-2958 and the companion galaxy with which it is interacting, both ultra luminous in the infrared, have been the subject of much attention in recent years, as the quasar host galaxy remained undetected. This led to various…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 G. Letawe , P. Magain

We have compared the B-V colour excess, E(B-V), obtained for a sample of five optically visible massive YSOs both from diffuse interstellar bands (DIBs) in their spectra and from their optical continuum slopes. Our targets are HD 200775,…

Astrophysics · Physics 2015-06-24 Rene D. Oudmaijer , Graeme Busfield , Janet E. Drew

We present spatially-resolved K- and L-band spectra (at spectral resolution R = 230 and R = 60, respectively) of MWC 419, a Herbig Ae/Be star. The data were obtained simultaneously with a new configuration of the 85-m baseline Keck…

We present new mid-infrared spectra for a sample of 15 targets (1 FU Orionis object, 4 Herbig Ae stars, 5 T Tauri stars and 5 Vega type stars), obtained with the TIMMI2 camera at La Silla Observatory (ESO). Three targets are members of the…

Solar and Stellar Astrophysics · Physics 2015-05-13 O. Schuetz , G. Meeus , M. F. Sterzik , E. Peeters

This work presents a study of two Herbig Ae transitional discs, Oph IRS 48 and HD 169142; which both have reported rings in their dust density distributions. We use Keck-II/NIRC2 adaptive optics imaging observations in the L' filter (3.8…

We are in a golden era observing Young Stellar Objects (YSOs), protoplanetary disks, and substellar objects, crucial for understanding their formation and evolution. This Ph.D. thesis explores two binary systems. Firstly, we study an…

Solar and Stellar Astrophysics · Physics 2024-07-22 Pedro H. Nogueira

Young stars with masses 2-8 Suns, called the Herbig Ae and Be stars, often show a near-infrared excess too large to explain with a hydrostatically-supported circumstellar disk of gas and dust. At the same time the accretion flow carrying…

Solar and Stellar Astrophysics · Physics 2015-06-17 N. J. Turner , M. Benisty , C. P. Dullemond , S. Hirose

(abridged) In this work we present the results of an optical and IR study for the curious B[e] star CD-42 11721. This object has a doubtful evolutionary stage, being either a pre-main sequence star (HAeB[e]) or an evolved star (sgB[e]). Our…

The polarization of light across individual spectral lines contains information about the circumstellar environment on very small spatial scales. We have obtained a large number of high precision, high resolution spectropolarimetric…

Astrophysics · Physics 2009-11-13 D. M. Harrington , J. R. Kuhn

The inner parts of the hot discs surrounding massive young stellar objects (MYSOs) are still barely explored due to observational limitations in terms of angular resolution, scarcity of diagnostic lines and the embedded and rare nature of…

Astrophysics of Galaxies · Physics 2024-10-09 E. Koumpia , D. Sun , M. Koutoulaki , J. D. Ilee , W. -J. de Wit , R. D. Oudmaijer , A. J. Frost

Owing to its unusual location and its isolation, the nature of the high Galactic latitude O9.5Vp object HD93521 is still uncertain. We have collected X-ray and optical observations to characterize the star and its surroundings. X-ray images…

Solar and Stellar Astrophysics · Physics 2015-06-11 Gregor Rauw , Thierry Morel , Matthieu Palate

HD~5501, a hitherto little studied eclipsing binary with an early A-type primary, has been caught in a short-lived, astrophysically interesting phase of its binary evolution. Recent photometric and spectroscopic observations, including…

We present the first observations of hydrogen line emission detected around the B-type star HD 46487, a well-studied star in the CoRoT field of view. The emission is only evident in the H$\alpha$ line, for which the observed violet-red peak…

Solar and Stellar Astrophysics · Physics 2017-05-26 David G. Whelan , R. David Baker

We analyze the physical conditions and chemical composition of the photoionized Herbig-Haro object HH~514, which emerges from the proplyd 170-337 in the core of the Orion Nebula. We use high-spectral resolution spectroscopy from UVES at the…

Astrophysics of Galaxies · Physics 2022-05-25 J. E. Méndez-Delgado , C. Esteban , J. García-Rojas , W. J. Henney , .

Planet formation has been known for many years to be tied to the spatial distribution of gas and dust in disks around young stars. To constrain planet formation models, imaging observations of protoplanetary disks are required. In this…

Astrophysics · Physics 2016-08-30 C. Doucet , E. Pantin , P. O. Lagage , C. P. Dullemond

Studies on the circumstellar structures around evolved stars provide vital information on the evolution of the parent star and the properties of the local interstellar medium. In this work, we present the discovery and characterization of…

Solar and Stellar Astrophysics · Physics 2022-07-20 Z. T. Spetsieri , P. Boumis , A. Chiotellis , S. Akras , S. Derlopa , S. Shetye , D. M. A. Meyer , D. M. Bowman , V. V. Gvaramadze

HD 100546 is a well-studied Herbig Be star-disk system that likely hosts a close-in companion with compelling observational evidence for an embedded protoplanet at 68 AU. We present ALMA observations of the HD 100546 disk which resolve the…

The very close environments of young stars are the hosts of fundamental physical processes, such as planet formation, star-disk interactions, mass accretion, and ejection. The complex morphological structure of these environments has been…

Solar and Stellar Astrophysics · Physics 2015-05-19 S. Renard , F. Malbet , M. Benisty , E. Thiébaut , J. -P. Berger

We present the first detections of gas around a 2.1 Myr old debris disc-bearing intermediate-mass star, HD 44892. Gas is detected both in $^{12}$CO (2-1) emission through ALMA Band 6 observations and in absorption in Ca II K and H, seen…

Earth and Planetary Astrophysics · Physics 2025-12-24 Karolina M. Szewczyk , Olja Panić , Daniela P. Iglesias , Tim D. Pearce , James M. Miley

HD 213985 is an eccentric binary system with a post-AGB primary and a jet-launching secondary star. We confirm that the system photometric variability is likely due to obscuration by the inner edge of a circumbinary disc, similar to…

Solar and Stellar Astrophysics · Physics 2025-06-10 Krystian Ilkiewicz , Lea Planquart , Tomek Kaminski , Hans Van Winckel
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