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Ammonia emission of dense cores in the RMC
The Rosette molecular cloud complex is a well-known Galactic star forming region with a morphology pointing towards triggered star formation. The distribution of its young... -
Periodic flares in two 6.7GHz methanol masers
Periodicity in the 6.7GHz methanol maser sources is a rare phenomenon discovered during long-term monitoring programs. Understanding underlying processes leading to periodic... -
Maggie filament datacubes
The atomic phase of the interstellar medium plays a key role in the formation process of molecular clouds. Due to the line-of-sight confusion in the Galactic plane that is... -
Large scale [CII] emission from the OMC
The [CII] 158um far-infrared (FIR) fine-structure line is one of the dominant cooling lines of the star-forming interstellar medium (ISM). Hence [CII] emission originates in,... -
ATLASGAL deuteration of ammonia
Deuteration has been used as a tracer of the evolutionary phases of low- and high-mass star formation. The APEX Telescope Large Area Survey (ATLASGAL) provides an important... -
4 post-AGB stars datacubes
There is a class of binary post-AGB stars with a remarkable near-infrared excess that are surrounded by Keplerian or quasi-Keplerian disks and extended outflows composed of gas... -
The Serpens filament 13CO, C18O and C17O datacubes
The Serpens filament, a prominent elongated structure in a relatively nearby molecular cloud, is believed to be at an early evolutionary stage, so studying its physical and... -
IC 3476 Halpha image
We study the IB(s)m galaxy IC 3476 observed in the context of the Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE), a blind narrow-band H{alpha}+[NII] imaging... -
Orion B in 18 molecular tracers maps
Molecular hydrogen being unobservable in cold molecular clouds, the column density measurements of molecular gas currently rely either on dust emission observation in the far-IR... -
Prestellar cores H2D+ and N2H+ maps
The study of prestellar cores is critical as they set the initial conditions in star formation and determine the final mass of the stellar object. To date, several hypotheses... -
Starless cores CH_3_OH and c-C_3_H_2_ maps
The spatial distribution of molecules around starless cores is a powerful tool for studying the physics and chemistry governing the earliest stages of star formation. Our aim is... -
Giant molecular filament GMF54 images
Recent surveys of the Galactic plane in the dust continuum and CO emission lines reveal that large (>~50pc) and massive (>~10^5^M_{sun}) filaments, know as giant molecular... -
Musca APEX 12CO(2-1), 12CO(3-2) & 12CO(4-3) data
Observations with the Herschel Space Telescope have established that most star forming gas is organised in filaments, a finding that is supported by numerical simulations of the... -
W43-MM1 ALMA ^12^CO(2-1) datacube
The accretion history of protostars remains widely mysterious even though it represents one of the best ways to understand the protostellar collapse that leads to the formation... -
Giant Molecular Filament THOR datacubes
Molecular clouds form from the atomic phase of the interstellar medium. However, characterizing the transition between the atomic and the molecular interstellar medium (ISM) is... -
36GHz methanol lines from nearby galaxies
Methanol (CH_3_OH) is one of the most abundant interstellar molecules, offering a vast number of transitions to be studied, including many maser lines. However, while the... -
NGC 6334 filament with ALMA
Herschel imaging surveys of galactic interstellar clouds support a paradigm for low-mass star formation in which dense molecular filaments play a crucial role. The detailed... -
L1188 HCO+, 12CO and 13CO datacubes
In order to search for further observational evidence of cloud-cloud collisions in one of the promising candidates, L1188, we carried out observations of multiple molecular... -
Perpendicular HF map to the Orion Bar
The hydrogen fluoride (HF) molecule is seen in absorption in the interstellar medium (ISM) along many lines of sight. Surprisingly, it is observed in emission toward the Orion... -
Starless core L1521E chemical structure
We have obtained ~2.5x2.5 arcminute maps toward L1521E using the IRAM-30m telescope in transitions of various species, including C^17^O, CH_3_OH c-C_3_H_2_, CN, SO, H_2_CS, and...
