Observations of protoplanetary disk structures
SM Andrews - Annual Review of Astronomy and Astrophysics, 2020 - annualreviews.org
The disks that orbit young stars are the essential conduits and reservoirs of material for star
and planet formation. Their structures, meaning the spatial variations of the disk physical …
and planet formation. Their structures, meaning the spatial variations of the disk physical …
Evolution of debris disks
MC Wyatt - Annu. Rev. Astron. Astrophys., 2008 - annualreviews.org
Circumstellar dust exists around several hundred main sequence stars. For the youngest
stars, that dust could be a remnant of the protoplanetary disk. Mostly it is inferred to be …
stars, that dust could be a remnant of the protoplanetary disk. Mostly it is inferred to be …
The Spitzer c2d legacy results: star-formation rates and efficiencies; evolution and lifetimes
NJ Evans, MM Dunham, JK Jørgensen… - The Astrophysical …, 2009 - iopscience.iop.org
ABSTRACT The c2d Spitzer Legacy project obtained images and photometry with both
IRAC and MIPS instruments for five large, nearby molecular clouds. Three of the clouds …
IRAC and MIPS instruments for five large, nearby molecular clouds. Three of the clouds …
Rapid planetesimal formation in turbulent circumstellar disks
During the initial stages of planet formation in circumstellar gas disks, dust grains collide and
build up larger and larger bodies. How this process continues from metre-sized boulders to …
build up larger and larger bodies. How this process continues from metre-sized boulders to …
The Disk Substructures at High Angular Resolution Project (DSHARP). V. Interpreting ALMA maps of protoplanetary disks in terms of a dust model
Abstract The Disk Substructures at High Angular Resolution Project (DSHARP) is the largest
homogeneous high-resolution (∼ 0 farcs 035, or∼ 5 au) disk continuum imaging survey …
homogeneous high-resolution (∼ 0 farcs 035, or∼ 5 au) disk continuum imaging survey …
Dust and gas in the disk of HL Tauri: surface density, dust settling, and dust-to-gas ratio
C Pinte, WRF Dent, F Ménard, A Hales… - The Astrophysical …, 2015 - iopscience.iop.org
The recent ALMA observations of the disk surrounding HL Tau reveal a very complex dust
spatial distribution. We present a radiative transfer model accounting for the observed gaps …
spatial distribution. We present a radiative transfer model accounting for the observed gaps …
The growth mechanisms of macroscopic bodies in protoplanetary disks
J Blum, G Wurm - Annu. Rev. Astron. Astrophys., 2008 - annualreviews.org
The formation of planetesimals, the kilometer-sized planetary precursors, is still a puzzling
process. Considerable progress has been made over the past years in the physical …
process. Considerable progress has been made over the past years in the physical …
Circumstellar dust disks in Taurus-Auriga: the submillimeter perspective
We present a sensitive, multiwavelength submillimeter continuum survey of 153 young
stellar objects in the Taurus-Auriga star formation region. The submillimeter detection rate is …
stellar objects in the Taurus-Auriga star formation region. The submillimeter detection rate is …
[BOOK][B] Astrophysics of planet formation
PJ Armitage - 2020 - books.google.com
" The study of planet formation has a long history. The idea that the Solar System formed
from a rotating disk of gas and dust-the Nebula Hypothesis-dates back to the writings of …
from a rotating disk of gas and dust-the Nebula Hypothesis-dates back to the writings of …
Resolved images of large cavities in protoplanetary transition disks
Circumstellar disks are thought to experience a rapid" transition" phase in their evolution that
can have a considerable impact on the formation and early development of planetary …
can have a considerable impact on the formation and early development of planetary …