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Nobeyama 45m Cygnus-X CO. II. C180 clumps
We report the statistical physical properties of the C^18^O(J=1-0) clumps present in a prominent cluster-forming region, Cygnus X, using the data set obtained by the Nobeyama... -
ALMA obs. toward NGC 5253. I. Molecular clouds
We present high-spatial-resolution (~0.2", or ~3pc) CO(2-1) observations of the nearest young starburst dwarf galaxy, NGC 5253, taken with the Atacama Large... -
A^1^{Pi}-X^1^{Sigma}^+^ transitions of CO study
Highly correlated ab initio calculations were performed for an accurate determination of the A^1^{Pi}-X^1^{Sigma}^+^ system of the CO molecule. A highly accurate multi-reference... -
Unlocking CO depletion in protoplanetary disks. I.
CO is commonly used as a tracer of the total gas mass in both the interstellar medium and in protoplanetary disks. Recently, there has been much debate about the utility of CO... -
Interferometric CO obs. of 126 CALIFA galaxies
We present interferometric CO observations, made with the Combined Array for Millimeter-wave Astronomy (CARMA) interferometer, of galaxies from the Extragalactic Database for... -
Molecular clouds in the dwarf galaxy NGC6822
We present the Atacama Large Millimeter/submillimeter Array survey of CO(2-1) emission from the 1/5 solar metallicity, Local Group dwarf galaxy NGC 6822. We achieve high... -
The PAWS catalogs of GMCs and islands in M51
Using data from the PdBI Arcsecond Whirlpool Survey (PAWS), we have generated the largest extragalactic giant molecular cloud (GMC) catalog to date, containing 1507 individual... -
CO and HCN observations of circumstellar envelopes
We have searched the literature for all observations of the ^12^CO(1-0), ^12^CO(2-1), and HCN(1-0) lines in circumstellar envelopes of late type stars published between January... -
13CO clump properties two 2 W5 bubble regions
The feedback effect of massive stars can either accelerate or inhibit star formation activity within molecular clouds. Studying the morphology of molecular clouds near W5 offers... -
12CO and HCN datacubes of NGC 253
Investigating molecular gas tracers, such as hydrogen cyanide (HCN), to probe higher densities than CO emission across nearby galaxies remains challenging. This is due to the... -
Sz 65 and Sz 66 ALMA observations
Substructures in disc density are ubiquitous in the bright extended discs that are observed with high resolution. These substructures are intimately linked to the physical... -
H2 in the diffuse ISM
Carbon monoxide (CO) is a poor tracer of H_2_ in the diffuse interstellar medium (ISM), where most of the carbon is not incorporated into CO molecules, unlike the situation at... -
IRAM NOEMA CO(1-0) cubes for IC342
We present a new wide-field 10.75x10.75arcmin^2^ (~11x11kpc^2^), high-resolution (theta=3.6"~60pc) NOEMA CO(1-0) survey of the very nearby (d=3.45Mpc) spiral galaxy IC 342. The... -
Horsehead ALMA images
Massive stars can determine the evolution of molecular clouds by eroding and photo-evaporating their surfaces with strong ultraviolet (UV) radiation fields. Moreover, UV... -
G333 giant molecular cloud complex moment maps
Hub-filament systems are suggested to be the birth cradles of high-mass stars and clusters. We investigate the gas kinematics of hub-filament structures in the G333 giant... -
Polaris Flare CO enhancement by MHD waves
The formation of molecular gas in interstellar clouds is a slow process, but can be enhanced by gas compression. Magnetohydrodynamic (MHD) waves can create compressed... -
Orion B molecular cloud CO and HCO datacubes
Recent Herschel observations of nearby molecular clouds have shown that filamentary structures are ubiquitous and that most prestellar cores form in dense filaments. Probing the... -
VERTICO III. Virgo cluster galaxies
In this Virgo Environment Traced in CO (VERTICO) science paper, we aim to study how the star formation process depends on the galactic environment and gravitational interactions... -
CO in the ALMA Radio-source Catalogue (ARC)
To evaluate the role of radio activity in galaxy evolution, we designed a large archival CO survey of radio galaxies (RGs) to determine their molecular gas masses at different... -
Post-common-envelope PN and mol. mass
Most planetary nebulae (PNe) show beautiful, axisymmetric morphologies despite their progenitor stars being essentially spherical. Close binarity is widely invoked to help eject...
