Results 151 to 160 of about 77,803 (191)
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy. [PDF]
Klaassen P +40 more
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Fundamentals of Interior Modelling and Challenges in the Interpretation of Observed Rocky Exoplanets. [PDF]
Baumeister P +9 more
europepmc +1 more source
The dramatic transition of the extreme Red Supergiant WOH G64 to a Yellow Hypergiant
Munoz-Sanchez G +10 more
europepmc +1 more source
Gravitational Instabilities in Circumstellar Disks [PDF]
ARAA Chapter to be published in Fall 2016.
Kaitlin Kratter, Giuseppe Lodato
exaly +3 more sources
Circumstellar disks around Herbig Be stars
Aims: Our goal is to investigate the properties of the circumstellar disks around intermediate mass stars to determine their occurrence, lifetime and evolution.
Asuncion Fuente +2 more
exaly +2 more sources
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Observations of Circumstellar Disks
Astrophysics and Space Science, 2004This review presents recent results on protoplanetary disks obtained from angularly resolved observations. Observations with mm arrays show that disks are in Keplerian rotation, with radius as large as 1000 AU. Optical images show disks to be flared.
Anne Dutrey, Stéphane Guilloteau
openaire +1 more source
A Circumstellar Disk Around β Pictoris
Science, 1984A circumstellar disk has been observed optically around the fourth-magnitude star β Pictoris. First detected in the infrared by the Infrared Astronomy Satellite last year, the disk is seen to extend to more than 400 astronomical units from the star, or more than twice the distance measured in the infrared by the Infrared Astronomy Satellite.
B A, Smith, R J, Terrile
openaire +2 more sources
Annual Review of Astronomy and Astrophysics, 2001
▪ Abstract Dusty circumstellar disks in orbit around main-sequence stars were discovered in 1983 by the infrared astronomical satellite. It was the first time material that was not another star had been seen in orbit around a main-sequence star other than our Sun.
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▪ Abstract Dusty circumstellar disks in orbit around main-sequence stars were discovered in 1983 by the infrared astronomical satellite. It was the first time material that was not another star had been seen in orbit around a main-sequence star other than our Sun.
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Circumstellar and circumplanetary disks
2000This thesis studies disks in three astrophysical contexts: (1) protoplanetary disks; (2) the Edgeworth-Kuiper Belt; and (3) planetary rings. We derive hydrostatic, radiative equilibrium models of passive protoplanetary disks surrounding T Tauri and Herbig Ae/Be stars. Each disk is encased by an optically thin layer of superheated dust grains.
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