Results 91 to 100 of about 411,596 (264)

Analysis of star-disk interaction in young stellar systems

open access: yesEPJ Web of Conferences, 2014
We present preliminary results of the study of star-disk interaction in the classical T Tauri star V354 Mon, a member of the young stellar cluster NGC 2264.
Fonseca N.N.J.   +2 more
doaj   +1 more source

HST/ACS Images of the GG Tauri Circumbinary Disk

open access: yes, 2005
Hubble Space Telescope Advanced Camera for Surveys images of the young binary GG Tauri and its circumbinary disk in V and I bandpasses were obtained in 2002 and are the most detailed of this system to date.
A. R. Martel   +13 more
core   +1 more source

Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Characterization of the young star T CrA and its circumstellar environment [PDF]

open access: hybrid, 2023
E. Rigliaco   +17 more
openalex   +1 more source

FIRST DETECTION OF c-C3H2 IN A CIRCUMSTELLAR DISK [PDF]

open access: yes, 2013
We report the first detection of c-C3H2 in a circumstellar disk. The c-C3H2 J = 6–5 line (217.882 GHz) is detected and imaged through Atacama Large Millimeter Array (ALMA) Science Verification observations toward the disk around the Herbig Ae star HD ...
C. Qi   +3 more
semanticscholar   +1 more source

The deep eclipses of RW Aur revisited by long‐term photometric and spectroscopic monitoring

open access: yesAstronomische Nachrichten, Volume 345, Issue 4, May 2024.
Abstract RW Aurigae is a young stellar system containing a classical T Tauri star as the primary component. It shows deep, irregular dimmings, first detected in 2010. At the University Observatory Jena, we carried out optical follow‐up observations. We performed multiband (BVRI) photometry of the system with the Cassegrain‐Teleskop‐Kamera II and the ...
Oliver Lux   +2 more
wiley   +1 more source

Complex Structure around a Circumstellar Disk Caused by Interchange Instability

open access: yesThe Astrophysical Journal Letters
We perform a three-dimensional nonideal magnetohydrodynamic simulation of a strongly magnetized cloud core and investigate the complex structure caused by the interchange instability. This is the first simulation that does not use a central sink cell and
Masahiro N. Machida, Shantanu Basu
doaj   +1 more source

LIGHT CURVE TYPES OF CLASSIC T TAURI STARS

open access: yesOdessa Astronomical Publications, 2016
By using the archive photometric data’s obtained for a long time intervals we have carried out a master light curves of 28 classical T Tauri type stars. For the physical character of variability mainly 5 type light curves can be separated.
N. Z. Ismailov, H. N. Adygezalzade
doaj   +1 more source

The T Tauri star RY Tau as a case study of the inner regions of circumstellar dust disks [PDF]

open access: yes, 2007
We study the inner region of the circumstellar disk around the TTauri star RY Tau. Our aim is to find a physical description satisfying the available interferometric data, obtained with the mid-infrared interferometric instrument at the Very Large ...
A. A. Schegerer   +119 more
core   +1 more source

Rapid disappearance of a warm, dusty circumstellar disk [PDF]

open access: yesNature, 2012
Stars form with gaseous and dusty circumstellar envelopes, which rapidly settle into disks that eventually give rise to planetary systems. Understanding the process by which these disks evolve is paramount in developing an accurate theory of planet ...
C. Melis   +5 more
semanticscholar   +1 more source

Limitations of the modified blackbody fit method for determining molecular cloud properties

open access: yesAstronomische Nachrichten, Volume 345, Issue 4, May 2024.
Abstract Achieving a comprehensive understanding of the star and planet formation process is one of the fundamental tasks of astrophysics, requiring detailed knowledge of the physical conditions during the different phases of this process. During the earliest stages, that is, concerning physical processes in molecular clouds and filaments, the column ...
Niko Zielinski, Sebastian Wolf
wiley   +1 more source

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