Results 61 to 70 of about 7,087 (197)

Formation of Gaps in Self-gravitating Debris Disks by Secular Resonance in a Single-planet System. II. Toward a Self-consistent Model

open access: yesThe Astrophysical Journal, 2023
High-resolution observations of several debris disks reveal structures such as gaps and spirals, suggestive of gravitational perturbations induced by underlying planets.
Antranik A. Sefilian   +2 more
doaj   +1 more source

Observations, Modeling, and Theory of Debris Disks [PDF]

open access: yes, 2014
to appear in Protostars & Planets VI.
Matthews, Brenda C.   +4 more
openaire   +2 more sources

Abundances in Stars with Debris Disks [PDF]

open access: yesProceedings of the International Astronomical Union, 2013
AbstractWe present preliminary results of a detailed chemical abundance analysis for a sample of solar-type stars known to exhibit excess infrared emission associated with dusty debris disks. Our sample of 28 stars was selected based on results from the Formation and Evolution of Planetary Systems (FEPS) Spitzer Legacy Program, for the purpose of ...
Ritchey, Adam M.   +3 more
openaire   +2 more sources

AKARI?IRC Survey of Hot Debris Disks

open access: yes, 2009
As a result of IRAS observations, main-sequence stars that have circumstellar debris disks and thus show infrared excess have been discovered. Since debris disks are thought to be the final stage of planet formation, it is very important to investigate ...
Usuda, Tomonori   +31 more
core   +1 more source

Massive Debris Disks May Hinder Secular Stirring by Planetary Companions: An Analytic Proof of Concept

open access: yesThe Astrophysical Journal
Debris disks or exo-Kuiper belts, detected through their thermal or scattered emission from their dusty components, are ubiquitous around main-sequence stars.
Antranik A. Sefilian
doaj   +1 more source

The ALMA survey to Resolve exoKuiper belt Substructures (ARKS)

open access: yesAstronomy & Astrophysics
Context. Debris disks – collisionally sustained belts of dust and sometimes gas around main sequence stars – are remnants of planet formation processes and are found in systems ≳10 Myr old.
Zawadzki B.   +39 more
doaj   +1 more source

Evidence for Misalignment between Debris Disks and Their Host Stars

open access: yesThe Astrophysical Journal, 2023
We place lower limits on the obliquities between debris disks and their host stars for 31 systems by comparing their disk and stellar inclinations.
Spencer A. Hurt, Meredith A. MacGregor
doaj   +1 more source

Collisional Grooming of Debris Disks [PDF]

open access: yesAIP Conference Proceedings, 2009
5 pages, Conference proceedings, "Exoplanets and Disks: Their Formation and Diversity" Kailua-Kona, Hawaii, 9-12 March 2009.
Marc J. Kuchner   +4 more
openaire   +2 more sources

Transient dust in warm debris disks

open access: yes, 2012
Context. Debris disks trace remnant reservoirs of leftover planetesimals in planetary systems. In the past years, a handful of “warm” debris disks have been discovered in which emission in excess starts in the mid-infrared. An interesting subset of these
Th. Henning   +6 more
core   +1 more source

Frequencies of Warm Debris Disks Based on Point Source Catalogs of Spitzer, WISE, and Gaia

open access: yesThe Astronomical Journal
More than a thousand warm debris disks have been detected as infrared excess at mid-infrared wavelengths, and their frequencies have been obtained for various spectral types of stars.
Toshiyuki Mizuki   +3 more
doaj   +1 more source

Home - About - Disclaimer - Privacy