Prediction of the soft X-ray absorption along lines of sight through our Galaxy is crucial for
understanding the spectra of extragalactic sources, but requires a good estimate of the …

Cancers that appear pathologically similar often respond differently to the same drug
regimens. Methods to better match patients to drugs are in high demand. We demonstrate a …

The CORNISH project is the highest resolution radio continuum survey of the Galactic plane
to date. It is the 5 GHz radio continuum part of a series of multi-wavelength surveys that …

We report on the source Gaia 17bpi and identify it as a new, ongoing FU Ori–type outburst,
associated with a young stellar object. The optical light curve from Gaia exhibited a 3.5 mag …

In this paper, we present a database of class I methanol masers. The compiled information
from the available literature provides an open and fast access to the data on class I …

We describe a new mm-wave molecular-line map** survey of the southern Galactic Plane
and its first data releases. The Three-mm Ultimate Mopra Milky Way Survey (ThrUMMS) …

Accretion in young stellar objects (YSOs) is at least partially episodic, ie periods with high
accretion rates ('bursts') are interspersed by quiescent phases. These bursts manifest …

Context. The formation process of high-mass stars (with masses> 8 M⊙) is still poorly
understood, and represents a challenge from both the theoretical and observational points …

We present new JVLA observations of the high-mass cluster-forming region W51A from 2 to
16 GHz with resolution θ fwhm≈ 0.3− 0.5 ″. The data reveal a wealth of observational …

We present a detailed analysis of the protostellar outflow activity in the massive star-forming
region NGC 3324, as revealed by new Early Release Observations (EROs) from the James …