An observational perspective of transitional disks
C Espaillat, J Muzerolle, J Najita, S Andrews… - arXiv preprint arXiv …, 2014 - arxiv.org
Transitional disks are objects whose inner disk regions have undergone substantial
clearing. The Spitzer Space Telescope produced detailed spectral energy distributions …
clearing. The Spitzer Space Telescope produced detailed spectral energy distributions …
A spectroscopic survey of Herbig Ae/Be stars with X-shooter–I. Stellar parameters and accretion rates
JR Fairlamb, RD Oudmaijer, I Mendigutia… - Monthly Notices of …, 2015 - academic.oup.com
Abstract Herbig Ae/Be stars (HAeBes) span a key mass range that links low-and high-mass
stars, and thus provide an ideal window from which to explore their formation. This paper …
stars, and thus provide an ideal window from which to explore their formation. This paper …
Sulphur monoxide emission tracing an embedded planet in the HD 100546 protoplanetary disk
Molecular line observations are powerful tracers of the physical and chemical conditions
across the different evolutionary stages of star, disk, and planet formation. The high angular …
across the different evolutionary stages of star, disk, and planet formation. The high angular …
Volatile-carbon locking and release in protoplanetary disks-A study of TW Hya and HD 100546
M Kama, S Bruderer, EF Van Dishoeck… - Astronomy & …, 2016 - aanda.org
Aims. The composition of planetary solids and gases is largely rooted in the processing of
volatile elements in protoplanetary disks. To shed light on the key processes, we carry out a …
volatile elements in protoplanetary disks. To shed light on the key processes, we carry out a …
The warm gas atmosphere of the HD 100546 disk seen by Herschel-Evidence of a gas-rich, carbon-poor atmosphere?
S Bruderer, EF van Dishoeck, SD Doty… - Astronomy & …, 2012 - aanda.org
Context. With the Herschel Space Observatory, lines of simple molecules (C+, O, and high-J
lines of CO, J up≳ 14) have been observed in the atmosphere of protoplanetary disks. When …
lines of CO, J up≳ 14) have been observed in the atmosphere of protoplanetary disks. When …
Flaring vs. self-shadowed disks: The SEDs of Herbig Ae/Be stars
CP Dullemond, C Dominik - Astronomy & Astrophysics, 2004 - aanda.org
Isolated Herbig Ae stars can be divided into two groups (Meeus et al. 2001): those with an
almost flat spectral energy distribution in the mid-infrared (“group I”), and those with a strong …
almost flat spectral energy distribution in the mid-infrared (“group I”), and those with a strong …
Structures in the protoplanetary disk of HD142527 seen in polarized scattered light
H Avenhaus, SP Quanz, HM Schmid… - The Astrophysical …, 2014 - iopscience.iop.org
We present H-and K s-band polarized differential images of the Herbig Ae/Be star
HD142527, revealing its optically thick outer disk and the nearly empty gap. The very small …
HD142527, revealing its optically thick outer disk and the nearly empty gap. The very small …
Small vs. large dust grains in transitional disks: do different cavity sizes indicate a planet?-SAO 206462 (HD 135344B) in polarized light with VLT/NACO
Context. Transitional disks represent a short stage of the evolution of circumstellar material.
Studies of dust grains in these objects can provide pivotal information on the mechanisms of …
Studies of dust grains in these objects can provide pivotal information on the mechanisms of …
The burst mode of protostellar accretion
EI Vorobyov, S Basu - The Astrophysical Journal, 2006 - iopscience.iop.org
We present new numerical simulations in the thin disk approximation that characterize the
burst mode of protostellar accretion. The burst mode begins upon the formation of a …
burst mode of protostellar accretion. The burst mode begins upon the formation of a …
A young protoplanet candidate embedded in the circumstellar disk of HD 100546
We present high-contrast observations of the circumstellar environment of the Herbig Ae/Be
star HD 100546. The final 3.8 μm image reveals an emission source at a projected …
star HD 100546. The final 3.8 μm image reveals an emission source at a projected …