Results 51 to 60 of about 7,087 (197)
Directly Imaging Circumstellar Debris Disks
: Debris disks are a collection of dust grains and planetesimals around a star and are thought to contain the remnants of planet formation. Directly imaging debris disks and studying their morphologies is valuable for studying the planet formation ...
core
JWST/NIRCam Detection of the Fomalhaut C Debris Disk in Scattered Light
Observations of debris disks offer important insights into the formation and evolution of planetary systems. Though M dwarfs make up approximately 80% of nearby stars, very few M dwarf debris disks have been studied in detail—making it unclear how or if ...
Kellen Lawson +22 more
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Giant Impacts and Debris Disk Morphology
Certain debris disks have nonaxisymmetric shapes in scattered light which are unexplained. The appearance of a disk depends on how its constituent Keplerian ellipses are arranged.
Joshua W. Jones +4 more
doaj +1 more source
Decay of Planetary Debris Disks [PDF]
We report new Spitzer 24 m photometry of 76 main-sequence A-type stars. We combine these results with previously reportedSpitzer24 m data and 24 and 25 m photometry from theInfrared Space Observatoryand the InfraredAstronomySatellite.Theresultisasampleof266starswithmasscloseto2.5M ,alldetectedtoatleastthe 7 level relative to their ...
G. H. Rieke +11 more
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Millimeter Studies of Nearby Debris Disks
At least 20% of nearby main sequence stars are known to be surrounded by disks of dusty material resulting from the collisional erosion of planetesimals, similar to asteroids and comets in our own Solar System.
MacGregor, Meredith Ann (5144465) +1 more
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MIRI MRS Observations of β Pictoris. I. The Inner Dust, the Planet, and the Gas
We present JWST MIRI Medium Resolution Spectrograph (MRS) observations of the β Pictoris system. We detect an infrared excess from the central unresolved point source from 5 to 7.5 μ m which is indicative of dust within the inner ∼7 au of the system.
Kadin Worthen +17 more
doaj +1 more source
Observations of circumstellar disks in scattered light with SPHERE at the VLT
The technological developments initiated in the early 21$^{\rm st}$ century have led to the implementation of “planet finders” instruments on 8-m class telescopes which are in operation since 2014-2015. Such facilities are at the inception of significant
Boccaletti, Anthony
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On the solar system—debris disk connection [PDF]
AbstractThis paper emphasizes the connection between solar and extra-solar debris disks: how models and observations of the Solar System are helping us understand the debris disk phenomenon, and vice versa, how debris disks are helping us place our Solar System into context.
openaire +2 more sources
The Edgeworth-Kuiper debris disk [PDF]
18 pages, 14 figures, accepted for publication in A& ...
Vitense, Christian +2 more
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β Pictoris's well-studied debris disk and two known giant planets, in combination with the stability of the Hubble Space Telescope’s Space Telescope Imaging Spectrograph (HST/STIS) (and now also JWST), offers a unique opportunity to test planet–disk ...
Arin M. Avsar +4 more
doaj +1 more source

