APOCENTER GLOW IN ECCENTRIC DEBRIS DISKS: IMPLICATIONS FOR FOMALHAUT AND
Debris disks often take the form of eccentric rings with azimuthal asymmetries in surface brightness. Such disks are often described as showing "pericenter glow," an enhancement of the disk brightness in regions nearest the central star. At long wavelengths, however, the disk apocenters sh...
Main Authors: | Pan, Margaret (Contributor), Nesvold, Erika R. (Author), Kuchner, Marc J. (Author) |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor) |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2017-06-13T14:58:02Z.
|
Subjects: | |
Online Access: | Get fulltext |
Similar Items
-
A Complete ALMA Map of the Fomalhaut Debris Disk
by: MacGregor, Meredith A., et al.
Published: (2017) -
A Complete ALMA Map of the Fomalhaut Debris Disk
by: MacGregor, Meredith A., et al.
Published: (2017) -
On the Dynamical System of Fomalhaut's Planet and Debris Disc
by: Yuan-Chen Wu, et al.
Published: (2013) -
MODERATE AND LOW PRESSURE GLOW DISCHARGE IN THE GAP BETWEEN TWO ECCENTRIC TUBES
by: Golovitskii Alexander, et al.
Published: (2021-03-01) -
The Dynamics and Implications of Gap Clearing via Planets in Planetesimal (Debris) Disks
by: Morrison, Sarah Jane, et al.
Published: (2017)