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LEGO II. 3mm molecular line study
The current generation of (sub)mm-telescopes have allowed molecular line emission to become a major tool for studying the physical, kinematic, and chemical properties of... -
Distances to molecular clouds in fourth quadrant
Distance measurements to molecular clouds are essential and important. We present directly measured distances to 169 molecular clouds in the fourth quadrant of the Milky Way.... -
JINGLE IV Dust in the local Universe
Scaling laws of dust, HI gas, and metal mass with stellar mass, specific star formation rate, and metallicity are crucial to our understanding of the build-up of galaxies... -
ATOMS II Compact objects in ACA observations
We report studies of the relationships between the total bolometric luminosity (L_bol_ or L_TIR_) and the molecular line luminosities of J=1-0 transitions of H^13^CN,... -
ATOMS I Description and a first look at G9.62+0.19
The ATOMS, standing for ALMA Three-millimeter Observations of Massive Star-forming regions, survey has observed 146 active star-forming regions with ALMA band 3, aiming to... -
MALATANG survey NGC253 dense gas & SFR formation
In order to study the high-transition dense-gas tracers and their relationships to the star formation of the inner ~2kpc circumnuclear region of NGC 253, we present HCN J=4-3... -
Crystalline silicate absorption at 11.1{mu}m
Utilizing several instruments on 4-8m telescopes, we have observed a large sample of objects in the mid-infrared (8-13{mu}m). These comprise a few evolved stars, multiple... -
A large catalogue of molecular clouds
We present a large, homogeneous catalogue of molecular clouds within 4kpc from the Sun at low Galactic latitudes (|b|<10{deg}) with unprecedented accurate distance... -
Dusty supernova remnants in the Galactic plane
We search for far-infrared (FIR) counterparts of known supernova remnants (SNRs) in the Galactic plane (360{deg} in longitude and b=+/-1{deg}) at 70-500{mu}m with Herschel. We... -
Aliphatic hydrocarbon within interstellar dust
In the interstellar medium, the cosmic elemental carbon abundance includes the total carbon in both gas and solid phases. The aim of the study was to trial a new method for... -
Ultracompact HII regions extended emission
In this paper, we present the results of a morphological study performed on a sample of 28 ultracompact HII (UC HII) regions located near extended free-free emission, using... -
JINGLE V Dust properties of nearby galaxies
We study the dust properties of 192 nearby galaxies from the JINGLE survey using photometric data in the 22-850{mu}m range. We derive the total dust mass, temperature T, and... -
Infall and outflow on massive star-forming regions
A total of 188 high-mass outflows have been identified from a sample of 694 clumps from the Millimetre Astronomy Legacy Team 90GHz survey, representing a detection rate of... -
Milky Way Project DR2 bubbles & bow shocks
Citizen science has helped astronomers comb through large data sets to identify patterns and objects that are not easily found through automated processes. The Milky Way Project... -
MIR spectra of AGNs heating molecular gas
We analyse 2015 mid-infrared (MIR) spectra of galaxies observed with Spitzer's Infrared Spectrograph, including objects with growing supermassive black holes (SMBHs) and objects... -
The SCOPE 850um compact source catalogue
We present the first release of the data and compact-source catalogue for the JCMT Large Program SCUBA-2 Continuum Observations of Pre-protostellar Evolution (SCOPE). SCOPE... -
Filaments hosting Planck Galactic cold clumps
We present a statistical study of the relative orientation in the plane of the sky between interstellar magnetic fields and filaments hosting cold clumps. For the first time, we... -
The gas-phase mass-metallicity relation
We present a detailed exploration of the stellar mass versus gas-phase metallicity relation (MZR) using integral field spectroscopy data obtained from ~1000 galaxies observed by... -
M33 dust-selected molecular cloud catalogue
We present a catalogue of Giant Molecular Clouds (GMCs) in M33, extracted from cold dust continuum emission. Our GMCs are identified by computing dendrograms. We measure the... -
AGN photoionization of gas in companion galaxies
We consider active galactic nucleus (AGN) photoionization of gas in companion galaxies (cross-ionization) as a way to sample the intensity of AGN radiation in both direction and...