Results 11 to 20 of about 584,793 (309)
ALMA Observations of the HD 110058 Debris Disk [PDF]
We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of the young, gas-rich debris disk around HD 110058 at 0.″3–0.″6 resolution. The disk is detected in the 0.85 and 1.3 mm continuum, as well as the J = 2–1 and J = 3–2 transitions
A. Hales +9 more
semanticscholar +1 more source
Polarization from Aligned Dust Grains in the β Pic Debris Disk [PDF]
We present 870 μm Atacama Large Millimeter/submillimeter Array polarization observations of thermal dust emission from the iconic, edge-on debris disk β Pic.
C. Hull +10 more
semanticscholar +1 more source
Multiwavelength Vertical Structure in the AU Mic Debris Disk: Characterizing the Collisional Cascade [PDF]
Debris disks are scaled-up analogs of the Kuiper Belt in which dust is generated by collisions between planetesimals. In the collisional cascade model of debris disks, the dust lost to radiation pressure and winds is constantly replenished by grinding ...
D. Vizgan +11 more
semanticscholar +1 more source
A Detailed Characterization of HR 8799's Debris Disk with ALMA in Band 7 [PDF]
The exoplanetary system of HR 8799 is one of the rare systems in which multiple planets have been directly imaged. Its architecture is strikingly similar to that of the solar system, with the four imaged giant planets surrounding a warm dust belt ...
V. Faramaz +10 more
semanticscholar +1 more source
From Pebbles and Planetesimals to Planets and Dust: The Protoplanetary Disk–Debris Disk Connection [PDF]
The similar orbital distances and detection rates of debris disks and the prominent rings observed in protoplanetary disks suggest a potential connection between these structures. We explore this connection with new calculations that follow the evolution
J. Najita, S. Kenyon, B. Bromley
semanticscholar +1 more source
Resolving Structure in the Debris Disk around HD 206893 with ALMA [PDF]
Debris disks are tenuous, dusty belts surrounding main-sequence stars generated by collisions between planetesimals. HD 206893 is one of only two stars known to host a directly imaged brown dwarf orbiting interior to its debris ring, in this case at a ...
Ava Nederlander +9 more
semanticscholar +1 more source
A Deep Polarimetric Study of the Asymmetrical Debris Disk HD 106906 [PDF]
Located in the Lower Centaurus Crux group, HD 106906 is a young, binary stellar system. This system is unique among discovered systems in that it contains an asymmetrical debris disk, as well as an 11 M Jup planet companion, at a separation of ∼735 au ...
K. Crotts +18 more
semanticscholar +1 more source
ALMA Images the Eccentric HD 53143 Debris Disk [PDF]
We present ALMA 1.3 mm observations of the HD 53143 debris disk—the first infrared or millimeter image produced of this ∼1 Gyr old solar analog. Previous HST STIS coronagraphic imaging did not detect flux along the minor axis of the disk, which could ...
M. MacGregor +8 more
semanticscholar +1 more source
Extreme Variability of the V488 Persei Debris Disk [PDF]
V488 Persei is the most extreme debris disk known in terms of the fraction of the stellar luminosity it intercepts and reradiates. The infrared output of its disk is extremely variable, similar in this respect to the most variable disk known previously ...
G. Rieke, K. Su, C. Melis, A. Gáspár
semanticscholar +1 more source
A Layered Debris Disk around M Star TWA 7 in Scattered Light [PDF]
We have obtained Hubble Space Telescope (HST) coronagraphic observations of the circumstellar disk around M star TWA 7 using the Space Telescope Imaging Spectrograph (STIS) instrument in visible light.
B. Ren 任 +17 more
semanticscholar +1 more source

