Results 301 to 310 of about 80,201 (344)
Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn
Fujimoto S +45 more
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Tracing chemical depletion in evolved binaries hosting second-generation transition discs. [PDF]
Mohorian M +6 more
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A binary merger product as the direct progenitor of a Type II-P supernova
Niu* Z +17 more
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Feedback mechanisms stopping the star formation in a pair of massive galaxies in the early Universe
Pérez-González P +21 more
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SHARP Images of Young Stellar Objects
Astrophysics and Space Science, 1995We present high resolution infrared images of the pre-main sequence star V536 Aql and polarization maps of the reflection nebula IRN Cha observed with the SHARP camera on the ESO NTT. Extended structures are observed near V536 Aql. The polarization pattern of IRN Cha is typical of a centrally illuminated source but with a central band of anomalously ...
N. Ageorges, A. Eckart, R. Hofmann
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Oscillations in Young Stellar Objects
International Astronomical Union Colloquium, 2002AbstractWe report the discovery of periodicities in the light curve of the Herbig Ae star V346 Ori. We interpret these variations as the superposition of at least two signals with periods P1=42±6 min and P2=68±12 min resulting from stellar oscillations.
F.J.G. Pinheiro +5 more
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Disks around young stellar objects
Pramana, 2011By 1939, when Chandrasekhar’s classic monograph on the theory of Stellar Structure was published, although the need for recent star formation was fully acknowledged, no one had yet recognized an object that could be called a star in the process of being born.
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IRAS Colours of Young Stellar Objects
Publications of the Astronomical Society of Australia, 1991AbstractThe effects of including low quality IRAS flux data in colour-colour diagrams is investigated, with a view to identifying Young Stellar Objects from the IRAS database. Colour criteria to perform this task are derived.
M. Suters, W. Zealey
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Observations of Young Stellar Objects
1988After a brief description of the main properties of embedded protostellar sources, I investigate in some detail the hypothesis that CO bipolar flows are pushed by winds emanating from the infrared central sources associated with the molecular outflows.
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