Results 11 to 20 of about 210,786 (294)
The Study of Debris Disks with SPICA [PDF]
SPICA joint European/Japanese Workshop, 2009 Debris disks are evidence that stars harbor reservoirs of dust-producing plantesimals on spatial scales similar the solar system. Debris disks present a wide range of sizes and structural features and there is growing evidence that, in some cases, they might be the result of the dynamical perturbations of a massive planet. Our solar system also harbors
Amaya Moro-Martίn
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MOLECULAR GAS IN YOUNG DEBRIS DISKS [PDF]
The Astrophysical Journal, 2011 Accepted for publication in ApJ Letters, 8 pages, 3 figures, 1 tables (emulateapj style)
Moór, A. +9 more
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Observing planet-disk interaction in debris disks [PDF]
Astronomy & Astrophysics, 2012 Context. Structures in debris disks induced by planetdisk interaction are promising to provide valuable constraints on the existence and properties of embedded planets. Aims. We investigate the observability of structures in debris disks induced by planet-disk interaction. Methods.
Ertel, S., Wolf, S., Rodmann, J.
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Debris disks around M dwarfs: The Herschel DEBRIS survey [PDF]
Astronomy & AstrophysicsThe Herschel open-time key program Disc Emission via a Bias-free Reconnaissance in the Infrared and Sub-millimeter (DEBRIS) is an unbiased survey of the nearest ∼100 stars for each stellar type A-M observed with a uniform photometric sensitivity to search for cold debris disks around them.
Lestrade, J.-F. +9 more
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BINARIES AMONG DEBRIS DISK STARS [PDF]
The Astrophysical Journal, 2012 We have gathered a sample of 112 main-sequence stars with known debris disks. We collected published information and performed adaptive optics observations at Lick Observatory to determine if these debris disks are associated with binary or multiple stars.
Rodríguez, David R., Zuckerman, B.
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DIAGNOSING CIRCUMSTELLAR DEBRIS DISKS [PDF]
The Astrophysical Journal, 2010 Accepted for publication in the Astrophysical ...
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HERSCHEL OBSERVATIONS OF DUSTY DEBRIS DISKS [PDF]
The Astrophysical Journal, 2016 ABSTRACT We present results from two Herschel observing programs using the Photodetector Array Camera and Spectrometer. During three separate campaigns, we obtained Herschel data for 24 stars at 70, 100, and 160 μm. We chose stars that were already known or suspected to have circumstellar dust based on excess infrared (IR) emission ...
Laura Vican +6 more
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Planetesimals in Debris Disks [PDF]
, 2017 Planetesimals form in gas-rich protoplanetary disks around young stars. However, protoplanetary disks fade in about 10 Myr. The planetesimals (and also many of the planets) left behind are too dim to study directly. Fortunately, collisions between planetesimals produce dusty debris disks.
Youdin, Andrew N., Rieke, George H.
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Planet forming disks, debris disks and the Solar System [PDF]
, 2020 VLT instruments and ALMA with their high spatial resolution have revolutionized in the past five years our view and understanding of how disks turn into planetary systems. This talk will briefly outline our current understanding of the physical processes
Salama, F., Linnartz, H., Kamp, Inga
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Long-term Evolution of Warps in Debris Disks—Application to the Gyr-old System HD 202628
The Astrophysical Journal, 2023 We present the results of N -body simulations meant to reproduce the long-term effects of mutually inclined exoplanets on debris disks, using the HD 202628 system as a proxy.
Madison T. Brady +3 more
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