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 …

A snow-line is the region of a protoplanetary disk at which a major volatile, such as water or
carbon monoxide, reaches its condensation temperature. Snow-lines play a crucial role in …

Abstract SCUBA-2 is a 10 000-bolometer submillimetre camera on the James Clerk Maxwell
Telescope. The instrument commissioning was completed in 2011 September, and full …

We have conducted a homogeneous near-infrared (near-IR) spectroscopic survey of 33
objects with varying degrees of similarity to FU Orionis. Common spectroscopic features that …

In this paper, we examine the issue of characterizing the transport associated with
gravitational instabilities in relatively cold discs, discussing in particular the conditions under …

Close encounters between young stellar objects in star-forming clusters are expected to
markedly perturb circumstellar disks. Such events are witnessed in numerical simulations of …

This paper describes a new Heterodyne Array Receiver Program (HARP) and Auto-
Correlation Spectral Imaging System (ACSIS) that have recently been installed and …

Investigating the response of icy dust aggregates to water ice sublimation is essential for
understanding the formation and properties of planetesimals in protoplanetary discs …

The FU Orionis–type objects (FUors) are low-mass pre-main-sequence stars undergoing a
temporary but significant increase of mass accretion rate from the circumstellar disk onto the …

We have constructed a detailed radiative transfer disk model which reproduces the main
features of the spectrum of the outbursting young stellar object FU Orionis from~ 4000 Å to …